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Space debris

Space debris (also known as space junk, space pollution,[1] space waste, space trash, space garbage, or cosmic debris[2]) are defunct human-made objects in space—principally in Earth orbit—which no longer serve a useful function. These include derelict spacecraft—nonfunctional spacecraft and abandoned launch vehicle stages—mission-related debris, and particularly numerous in Earth orbit, fragmentation debris from the breakup of derelict rocket bodies and spacecraft. In addition to derelict human-made objects left in orbit, other examples of space debris include fragments from their disintegration, erosion and collisions or even paint flecks, solidified liquids expelled from spacecraft, and unburned particles from solid rocket motors. Space debris represents a risk to spacecraft.[3]

A computer-generated image representing the locations, but not relative sizes, of space debris as could be seen from high Earth orbit. The two main debris fields are the ring of objects in geosynchronous Earth orbit (GEO) and the cloud of objects in low Earth orbit (LEO).

Space debris is typically a negative externality—it creates an external cost on others from the initial action to launch or use a spacecraft in near-Earth orbit—a cost that is typically not taken into account nor fully accounted for in the cost[4][5] by the launcher or payload owner.[6][1][7]

Several spacecraft, both crewed and uncrewed, have been damaged or destroyed by space debris. The measurement, mitigation, and potential removal of debris are conducted by some participants in the space industry.[8]

As of November 2022, the US Space Surveillance Network reported 25,857 artificial objects in orbit above the Earth,[9] including 5,465 operational satellites.[10] However, these are just the objects large enough to be tracked and in an orbit that makes tracking possible. Satellite debris that is in a Molnya orbit, such as the Kosmos Ono series, might be too high above the northern hemisphere to be tracked.[11] As of January 2019, more than 128 million pieces of debris smaller than 1 cm (0.4 in), about 900,000 pieces of debris 1–10 cm, and around 34,000 of pieces larger than 10 cm (3.9 in) were estimated to be in orbit around the Earth.[8] When the smallest objects of artificial space debris (paint flecks, solid rocket exhaust particles, etc.) are grouped with micrometeoroids, they are together sometimes referred to by space agencies as MMOD (Micrometeoroid and Orbital Debris). Collisions with debris have become a hazard to spacecraft; the smallest objects cause damage akin to sandblasting, especially to solar panels and optics like telescopes or star trackers that cannot easily be protected by a ballistic shield.[12]

Below 2,000 km (1,200 mi) Earth-altitude, pieces of debris are denser than meteoroids; most are dust from solid rocket motors, surface erosion debris like paint flakes, and frozen coolant from Soviet nuclear-powered satellites.[13][14][15] For comparison, the International Space Station orbits in the 300–400 kilometres (190–250 mi) range, while the two most recent large debris events—the 2007 Chinese antisat weapon test and the 2009 satellite collision—occurred at 800 to 900 kilometres (500 to 560 mi) altitude.[16] The ISS has Whipple shielding to resist damage from small MMOD; however, known debris with a collision chance over 1/10,000 are avoided by maneuvering the station.

History

Space debris began to accumulate in Earth orbit immediately with the first launch of an artificial satellite Sputnik 1 into orbit in October 1957. But even before that humans might have produced ejecta that became space debris, as in the August 1957 Pascal B test.[17][18] Going back even earlier, there was natural ejecta from Earth in orbit.

After the launch of Sputnik, the North American Aerospace Defense Command (NORAD) began compiling a database (the Space Object Catalog) of all known rocket launches and objects reaching orbit: satellites, protective shields and upper-stages of launch vehicles. NASA later published modified versions of the database in two-line element set,[19] and beginning in the early 1980s the CelesTrak bulletin board system re-published them.[20]

 
Gabbard diagram of almost 300 pieces of debris from the disintegration of the five-month-old third stage of the Chinese Long March 4 booster on 11 March 2000

The trackers (NORAD) who fed the database were aware of other objects in orbit, many of which were the result of in-orbit explosions.[21] Some were deliberately caused during the 1960s anti-satellite weapon (ASAT) testing, and others were the result of rocket stages blowing up in orbit as leftover propellant expanded and ruptured their tanks. To improve tracking, NORAD employee John Gabbard kept a more detailed database of as many objects as he could identify.[22]

Studying the explosions, In March 1971, Gabbard developed a technique for predicting the orbital paths of their products, and Gabbard diagrams (or plots) are now widely used. These studies were used to improve the modeling of orbital evolution and decay.[23]

When the NORAD database became publicly available during the 1970s,[clarification needed] techniques developed for the asteroid-belt were applied to the study[by whom?] to the database of known artificial satellite Earth objects.[citation needed]

 
Baker-Nunn cameras were widely used to study space debris.

In addition to approaches to debris reduction where time and natural gravitational/atmospheric effects help to clear space debris, or a variety of technological approaches that have been proposed (with most not implemented) to reduce space debris, a number of scholars have observed that institutional factors—political, legal, economic and cultural "rules of the game"—are the greatest impediment to the cleanup of near-Earth space. By 2014, there was little commercial incentive to reduce space debris, since the cost of dealing with it is not assigned to the entity producing it, but rather falls on all users of the space environment, and rely on human society as a whole that benefits from space technologies and knowledge. A number of suggestions for improving institutions so as to increase the incentives to reduce space debris have been made. These include government mandates to create incentives, as well as companies coming to see economic benefit to reducing debris more aggressively than existing government standard practices.[24] In 1979 NASA founded the Orbital Debris Program to research mitigation measures for space debris in Earth orbit.[25][26]

Debris growth

During the 1980s, NASA and other U.S. groups attempted to limit the growth of debris. One trial solution was implemented by McDonnell Douglas in 1981 for the Delta launch vehicle, by having the booster move away from its payload and vent any propellant remaining in its tanks.[27] This eliminated one source for pressure buildup in the tanks which had previously caused them to explode and create additional orbital debris.[28] Other countries were slower to adopt this measure and, due especially to a number of launches by the Soviet Union, the problem grew throughout the decade.[29]

A new battery of studies followed as NASA, NORAD and others attempted to better understand the orbital environment, with each adjusting the number of pieces of debris in the critical-mass zone upward. Although in 1981 (when Schefter's article was published) the number of objects was estimated at 5,000,[21] new detectors in the Ground-based Electro-Optical Deep Space Surveillance system found new objects. By the late 1990s, it was thought that most of the 28,000 launched objects had already decayed and about 8,500 remained in orbit.[30] By 2005 this was adjusted upward to 13,000 objects,[31] and a 2006 study increased the number to 19,000 as a result of an ASAT and a satellite collision.[32] In 2011, NASA said that 22,000 objects were being tracked.[33]

A 2006 NASA model suggested that if no new launches took place the environment would retain the then-known population until about 2055, when it would increase on its own.[34][35] Richard Crowther of Britain's Defence Evaluation and Research Agency said in 2002 that he believed the cascade would begin about 2015.[36] The National Academy of Sciences, summarizing the professional view, noted widespread agreement that two bands of LEO space—900 to 1,000 km (620 mi) and 1,500 km (930 mi)—were already past critical density.[37]

In the 2009 European Air and Space Conference, University of Southampton researcher Hugh Lewis predicted that the threat from space debris would rise 50 percent in the next decade and quadruple in the next 50 years. As of 2009, more than 13,000 close calls were tracked weekly.[38]

A 2011 report by the U.S. National Research Council warned NASA that the amount of orbiting space debris was at a critical level. According to some computer models, the amount of space debris "has reached a tipping point, with enough currently in orbit to continually collide and create even more debris, raising the risk of spacecraft failures". The report called for international regulations limiting debris and research of disposal methods.[39]

 
Objects in Earth orbit including fragmentation debris. November 2020 NASA:ODPO

Debris history in particular years

  • By mid-1994 there had been 68 breakups or debris "anomalous events" involving satellites launched by the former Soviet Union/Russia and 18 similar events had been discovered involving rocket bodies and other propulsion-related operational debris.[40]
  • As of 2009, 19,000 debris over 5 cm (2 in) were tracked by United States Space Surveillance Network.[16]
  • As of July 2013, estimates of more than 170 million debris smaller than 1 cm (0.4 in), about 670,000 debris 1–10 cm, and approximately 29,000 larger pieces of debris are in orbit.[41]
  • As of July 2016, nearly 18,000 artificial objects are orbiting above Earth,[42] including 1,419 operational satellites.[43]
  • As of October 2019, nearly 20,000 artificial objects in orbit above the Earth,[9] including 2,218 operational satellites.[10]

Characterization

Size

There are estimated to be over 128 million pieces of debris smaller than 1 cm (0.39 in) as of January 2019. There are approximately 900,000 pieces from 1 to 10 cm. The current count of large debris (defined as 10 cm across or larger[44]) is 34,000.[8] The technical measurement cutoff[clarification needed] is c. 3 mm (0.12 in).[45] As of 2020, there are 8,000 metric tons of debris in orbit, a figure that is expected to increase.[46]

Low Earth orbit

 
Satellite hit by a space debris, animation by ESA

In the orbits nearest to Earth—less than 2,000 km (1,200 mi) orbital altitude, referred to as low-Earth orbit (LEO)—there have traditionally been few "universal orbits" that keep a number of spacecraft in particular rings (in contrast to GEO, a single orbit that is widely used by over 500 satellites). This is beginning to change in 2019, and several companies have begun to deploy the early phases of satellite internet constellations, which will have many universal orbits in LEO with 30 to 50 satellites per orbital plane and altitude. Traditionally, the most populated LEO orbits have been a number of sun-synchronous satellites that keep a constant angle between the Sun and the orbital plane, making Earth observation easier with consistent sun angle and lighting. Sun-synchronous orbits are polar, meaning they cross over the polar regions. LEO satellites orbit in many planes, typically up to 15 times a day, causing frequent approaches between objects. The density of satellites—both active and derelict—is much higher in LEO.[47]

Orbits are affected by gravitational perturbations (which in LEO include unevenness of the Earth's gravitational field due to variations in the density of the planet), and collisions can occur from any direction. The average impact speed of collisions in Low Earth Orbit is 10 km/s with maximums reaching above 14 km/s due to orbital eccentricity.[48] The 2009 satellite collision occurred at a closing speed of 11.7 km/s (26,000 mph),[49] creating over 2,000 large debris fragments.[50] These debris cross many other orbits and increase debris collision risk.

It is theorized that a sufficiently large collision of spacecraft could potentially lead to a cascade effect, or even make some particular low Earth orbits effectively unusable for long term use by orbiting satellites, a phenomenon known as the Kessler syndrome.[51] The theoretical effect is projected to be a theoretical runaway chain reaction of collisions that could occur, exponentially increasing the number and density of space debris in low-Earth orbit, and has been hypothesized to ensue beyond some critical density.[52]

Crewed space missions are mostly at 400 km (250 mi) altitude and below, where air drag helps clear zones of fragments. The upper atmosphere is not a fixed density at any particular orbital altitude; it varies as a result of atmospheric tides and expands or contracts over longer time periods as a result of space weather.[53] These longer-term effects can increase drag at lower altitudes; the 1990s expansion was a factor in reduced debris density.[54] Another factor was fewer launches by Russia; the Soviet Union made most of their launches in the 1970s and 1980s.[55]: 7 

Higher altitudes

At higher altitudes, where air drag is less significant, orbital decay takes longer. Slight atmospheric drag, lunar perturbations, Earth's gravity perturbations, solar wind and solar radiation pressure can gradually bring debris down to lower altitudes (where it decays), but at very high altitudes this may take centuries.[56] Although high-altitude orbits are less commonly used than LEO and the onset of the problem is slower, the numbers progress toward the critical threshold more quickly.[contradictory][page needed][57]

Many communications satellites are in geostationary orbits (GEO), clustering over specific targets and sharing the same orbital path. Although velocities are low between GEO objects, when a satellite becomes derelict (such as Telstar 401) it assumes a geosynchronous orbit; its orbital inclination increases about .8° and its speed increases about 160 km/h (99 mph) per year. Impact velocity peaks at about 1.5 km/s (0.93 mi/s). Orbital perturbations cause longitude drift of the inoperable spacecraft and precession of the orbital plane. Close approaches (within 50 meters) are estimated at one per year.[58] The collision debris pose less short-term risk than from an LEO collision, but the satellite would likely become inoperable. Large objects, such as solar-power satellites, are especially vulnerable to collisions.[59]

Although the ITU now requires proof a satellite can be moved out of its orbital slot at the end of its lifespan, studies suggest this is insufficient.[60] Since GEO orbit is too distant to accurately measure objects under 1 m (3 ft 3 in), the nature of the problem is not well known.[61] Satellites could be moved to empty spots in GEO, requiring less maneuvering and making it easier to predict future motion.[62] Satellites or boosters in other orbits, especially stranded in geostationary transfer orbit, are an additional concern due to their typically high crossing velocity.

Despite efforts to reduce risk, spacecraft collisions have occurred. The European Space Agency telecom satellite Olympus-1 was struck by a meteoroid on 11 August 1993 and eventually moved to a graveyard orbit.[63] On 29 March 2006, the Russian Express-AM11 communications satellite was struck by an unknown object and rendered inoperable;[64] its engineers had enough contact time with the satellite to send it into a graveyard orbit.

Sources

Dead spacecraft

 
Vanguard 1 is expected to remain in orbit for 240 years.[65][66]

In 1958, the United States launched Vanguard I into a medium Earth orbit (MEO). As of October 2009, it, the upper stage of its launch rocket and associated piece of debris, are the oldest surviving artificial space objects still in orbit and are expected to be until after the year 2250.[67][68] As of May 2022, the Union of Concerned Scientists listed 5,465 operational satellites from a known population of 27,000 pieces of orbital debris tracked by NORAD.[69][70]

While sometimes satellites are simply left in orbit when they're no longer useful, many countries require that satellites go through passivation at the end of their life. They are then either boosted into a higher, "graveyard" orbit or a lower, short-term orbit. But even satellites that have been properly moved to a higher orbit have an eight-percent probability of puncture and coolant release over a 50-year period. The coolant freezes into droplets of solid sodium-potassium alloy, creating more debris.[13][71]

Despite the use of passivization, or prior to its standardization, many satellites and rocket bodies have exploded or broken apart on orbit. In February 2015, for example, the USAF Defense Meteorological Satellite Program Flight 13 (DMSP-F13) exploded on orbit, creating at least 149 debris objects, which were expected to remain in orbit for decades.[72] Later that same year, NOAA-16 which had been decommissioned after an anomaly in June 2014, broke apart on orbit into at least 275 pieces.[73] For older programs, such as the Soviet-era Meteor 2 and Kosmos satellites, design flaws resulted in numerous break-ups - at least 68 by 1994 - following decommissioning, resulting in more debris.[40]

In addition to the accidental creation of debris, some has been made intentionally through the deliberate destruction of satellites. This has been done as a test of anti-satellite or anti-ballistic missile technology, or to prevent a sensitive satellite from being examined by a foreign power.[40] The United States has conducted over 30 anti-satellite weapons tests (ASATs), the Soviet Union/Russia has performed at least 27, China has performed 10 and India has performed at least one.[74][75] The most recent ASATs were the Chinese interception of FY-1C, Russian trials of its PL-19 Nudol, the American interception of USA-193 and India's interception of an unstated live satellite.[75]

Lost equipment

 
A drifting thermal blanket photographed in 1998 during STS-88.

Space debris includes a glove lost by astronaut Ed White on the first American space-walk (EVA), a camera lost by Michael Collins near Gemini 10, a thermal blanket lost during STS-88, garbage bags jettisoned by Soviet cosmonauts during Mir's 15-year life,[76] a wrench, and a toothbrush.[77] Sunita Williams of STS-116 lost a camera during an EVA. During an STS-120 EVA to reinforce a torn solar panel, a pair of pliers was lost, and in an STS-126 EVA, Heidemarie Stefanyshyn-Piper lost a briefcase-sized tool bag.[78]

Boosters

 
Spent upper stage of a Delta II rocket, photographed by the XSS 10 satellite

Rocket upper stages which end up in orbit are a significant source of space debris. In characterizing the problem of space debris, it was learned that much debris was due to rocket upper stages (e.g. the Inertial Upper Stage) which end up in orbit, and break up due to decomposition of unvented unburned fuel.[79] The first such instance involved the launch of the Transit-4a satellite in 1961. Two hours after insertion the Ablestar upper stage exploded. But even boosters that don't break apart can be a problem as a major known impact event involved an (intact) Ariane booster.[55]: 2 

Although NASA and the United States Air Force now require upper-stage passivation, other launchers - such as the Chinese and Russian space agencies - do not. Lower stages, like the Space Shuttle's solid rocket boosters or Apollo program's Saturn IB launch vehicles, do not reach orbit.[80]

 
Orbit of 2020 SO

Examples:

  • Two Japanese H-2A rockets rockets broke up in 2006.[81]
  • A Russian Briz-M booster stage exploded in orbit over South Australia on 19 February 2007. Launched on 28 February 2006 carrying an Arabsat-4A communications satellite, it malfunctioned before it could use up its propellant. Although the explosion was captured on film by astronomers, due to the orbit path the debris cloud has been difficult to measure with radar. By 21 February 2007, over 1,000 fragments were identified.[82][83] A 14 February 2007 breakup was recorded by Celestrak.[84]
  • Another Briz-M broke up on 16 October 2012 after a failed 6 August Proton-M launch. The amount and size of the debris was unknown.[85]
  • The second stage of the Zenit-2, called the SL-16 by western governments, along with the second stages of the Vostok and Kosmos launch vehicles, make up about 20% of the total mass of launch debris in Low Earth Orbit (LEO).[86] An analysis that determined the 50 “statistically most concerning” debris objects in low Earth orbit determined that the top 20 were all Zenit-2 upper stages.[87]
  • a Delta II rocket used to launch NASA’s 1989 COBE spacecraft exploded on December 3, 2006. This occurred even though its residual fuel had already been vented to space.[81]
  • In 2018–2019, three different Atlas V Centaur second stages broke up.[88][89][90]
  • In December 2020, scientists confirmed that a previously detected near-Earth object, 2020 SO, was rocket booster space junk launched in 1966 orbiting Earth and the Sun.[91]
  • At least eight Delta rockets have contributed orbital debris in the sun-synchronous low earth orbit environment. The variant of the Delta upper stage that was used in the 1970's was found to be prone to in-orbit explosions. Starting in 1981, depletion burns - to get rid of excess propellant - became standard and no Delta Rocket Bodies launched after 1981 experience severe fragmentations afterward, but some of those launched prior to 1981 continued to explode. In 1991, the Delta 1975-052B fragmented, 16 years after launch, demonstrating the resilience of the propellent.[92]

Weapons

A past debris source was the testing of anti-satellite weapons (ASATs) by the U.S. and Soviet Union during the 1960s and 1970s. North American Aerospace Defense Command (NORAD) files only contained data for Soviet tests, and debris from U.S. tests were only identified later.[93] By the time the debris problem was understood, widespread ASAT testing had ended; the U.S. Program 437 was shut down in 1975.[94]

The U.S. restarted their ASAT programs in the 1980s with the Vought ASM-135 ASAT. A 1985 test destroyed a 1-tonne (2,200 lb) satellite orbiting at 525 km (326 mi), creating thousands of debris larger than 1 cm (0.39 in). Due to the altitude, atmospheric drag decayed the orbit of most debris within a decade. A de facto moratorium followed the test.[95]

 
Known orbit planes of Fengyun-1C debris one month after the weather satellite's disintegration by the Chinese ASAT

China's government was condemned for the military implications and the amount of debris from the 2007 anti-satellite missile test,[96] the largest single space debris incident in history (creating over 2,300 pieces golf-ball size or larger, over 35,000 1 cm (0.4 in) or larger, and one million pieces 1 mm (0.04 in) or larger). The target satellite orbited between 850 km (530 mi) and 882 km (548 mi), the portion of near-Earth space most densely populated with satellites.[97] Since atmospheric drag is low at that altitude, the debris is slow to return to Earth, and in June 2007 NASA's Terra environmental spacecraft maneuvered to avoid impact from the debris.[98] Dr. Brian Weeden, U.S. Air Force officer and Secure World Foundation staff member, noted that the 2007 Chinese satellite explosion created an orbital debris of more than 3,000 separate objects that then required tracking.[99] On 20 February 2008, the U.S. launched an SM-3 missile from the USS Lake Erie to destroy a defective U.S. spy satellite thought to be carrying 450 kg (1,000 lb) of toxic hydrazine propellant. The event occurred at about 250 km (155 mi), and the resulting debris has a perigee of 250 km (155 mi) or lower.[100] The missile was aimed to minimize the amount of debris, which (according to Pentagon Strategic Command chief Kevin Chilton) had decayed by early 2009.[101]

On 27 March 2019, Indian Prime Minister Narendra Modi announced that India shot down one of its own LEO satellites with a ground-based missile. He stated that the operation, part of Mission Shakti, would defend the country's interests in space. Afterwards, US Air Force Space Command announced they were tracking 270 new pieces of debris but expected the number to grow as data collection continues.[102]

On 15 November 2021, the Russian Defense Ministry destroyed Kosmos 1408[103] orbiting at around 450 km, creating "more than 1,500 pieces of trackable debris and hundreds of thousands of pieces of un-trackable debris" according to the US State Department.[104]

The vulnerability of satellites to debris and the possibility of attacking LEO satellites to create debris clouds has triggered speculation that it is possible for countries unable to make a precision attack.[clarification needed] An attack on a satellite of 10 t (22,000 lb) or more would heavily damage the LEO environment.[95]

Hazards

 
A micrometeoroid left this crater on the surface of Space Shuttle Challenger's front window on STS-7.

To spacecraft

Space junk can be a hazard to active satellites and spacecraft. It has been theorized that Earth orbit could even become impassable if the risk of collision grows too high.[105][failed verification]

However, since the risk to spacecraft increases with exposure to high debris densities, it is more accurate to say that LEO would be rendered unusable by orbiting craft. The threat to craft passing through LEO to reach a higher orbit would be much lower owing to the very short time span of the crossing.

Uncrewed spacecraft

Although spacecraft are typically protected by Whipple shields, solar panels, which are exposed to the Sun, wear from low-mass impacts. Even small impacts can produce a cloud of plasma which is an electrical risk to the panels.[106]

Satellites are believed to have been destroyed by micrometeorites and (small) orbital debris (MMOD). The earliest suspected loss was of Kosmos 1275, which disappeared on 24 July 1981 (a month after launch). Kosmos contained no volatile fuel, therefore, there appeared to be nothing internal to the satellite which could have caused the destructive explosion which took place. However, the case has not been proven and another hypothesis forwarded is that the battery exploded. Tracking showed it broke up, into 300 new objects.[107]

Many impacts have been confirmed since. For example, on 24 July 1996, the French microsatellite Cerise was hit by fragments of an Ariane-1 H-10 upper-stage booster which exploded in November 1986.[55]: 2  On 29 March 2006, the Russian Ekspress AM11 communications satellite was struck by an unknown object and rendered inoperable.[64] On 13 October 2009, Terra suffered a single battery cell failure anomaly and a battery heater control anomaly which were subsequently considered likely the result of an MMOD strike.[108] On 12 March 2010, Aura lost power from one-half of one of its 11 solar panels and this was also attributed to an MMOD strike.[109] On 22 May 2013, GOES 13 was hit by an MMOD which caused it to lose track of the stars that it used to maintain an operational attitude. It took nearly a month for the spacecraft to return to operation.[110]

The first major satellite collision occurred on 10 February 2009. The 950 kg (2,090 lb) derelict satellite Kosmos 2251 and the operational 560 kg (1,230 lb) Iridium 33 collided, 500 mi (800 km)[111] over northern Siberia. The relative speed of impact was about 11.7 km/s (7.3 mi/s), or about 42,120 km/h (26,170 mph).[112] Both satellites were destroyed, creating thousands of pieces of new smaller debris, with legal and political liability issues unresolved even years later.[113][114][115] On 22 January 2013, BLITS (a Russian laser-ranging satellite) was struck by debris suspected to be from the 2007 Chinese anti-satellite missile test, changing both its orbit and rotation rate.[116]

Satellites sometimes[clarification needed] perform Collision Avoidance Maneuvers and satellite operators may monitor space debris as part of maneuver planning. For example, in January 2017, the European Space Agency made the decision to alter orbit of one of its three[117] Swarm mission spacecraft, based on data from the US Joint Space Operations Center, to lower the risk of collision from Cosmos-375, a derelict Russian satellite.[118]

Crewed spacecraft

Crewed flights are naturally particularly sensitive to the hazards that could be presented by space debris conjunctions in the orbital path of the spacecraft. Examples of occasional avoidance maneuvers, or longer-term space debris wear, have occurred in Space Shuttle missions, the MIR space station, and the International Space Station.

Space Shuttle missions
 
Space Shuttle Discovery's lower starboard wing and Thermal Protection System tiles, photographed on STS-114 during an R-Bar Pitch Manoeuvre where astronauts examine the TPS for any damage during ascent

From the early Space Shuttle missions, NASA used NORAD space monitoring capabilities to assess the Shuttle's orbital path for debris. In the 1980s, this used a large proportion of NORAD capacity.[28] The first collision-avoidance maneuver occurred during STS-48 in September 1991,[119] a seven-second thruster burn to avoid debris from the derelict satellite Kosmos 955.[120] Similar maneuvers were initiated on missions 53, 72 and 82.[119]

One of the earliest events to publicize the debris problem occurred on Space Shuttle Challenger's second flight, STS-7. A fleck of paint struck its front window, creating a pit over 1 mm (0.04 in) wide. On STS-59 in 1994, Endeavour's front window was pitted about half its depth. Minor debris impacts increased from 1998.[121]

Window chipping and minor damage to thermal protection system tiles (TPS) were already common by the 1990s. The Shuttle was later flown tail-first to take a greater proportion of the debris load on the engines and rear cargo bay, which are not used in orbit or during descent, and thus are less critical for post-launch operation. When flying attached to the ISS, the two connected spacecraft were flipped around so the better-armoured station shielded the orbiter.[122]

 
Space Shuttle Endeavour had a major impact on its radiator during STS-118. The entry hole is about 5.5 mm (0.22 in), and the exit hole is twice as large.

A NASA 2005 study concluded that debris accounted for approximately half of the overall risk to the Shuttle.[122][123] Executive-level decision to proceed was required if the catastrophic impact was likelier than 1 in 200. On a normal (low-orbit) mission to the ISS, the risk was approximately 1 in 300, but the Hubble telescope repair mission was flown at the higher orbital altitude of 560 km (350 mi) where the risk was initially calculated at a 1-in-185 (due in part to the 2009 satellite collision). A re-analysis with better debris numbers reduced the estimated risk to 1 in 221, and the mission went ahead.[124]

Debris incidents continued on later Shuttle missions. During STS-115 in 2006 a fragment of circuit board bored a small hole through the radiator panels in Atlantis's cargo bay.[125] On STS-118 in 2007 debris blew a bullet-like hole through Endeavour's radiator panel.[126]

Mir

Impact wear was notable on Mir, the Soviet space station since it remained in space for long periods with its original solar module panels.[127][128]

 
Debris impacts on Mir's solar panels degraded their performance. The damage is most noticeable on the panel on the right, which is facing the camera with a high degree of contrast. Extensive damage to the smaller panel below is due to impact with a Progress spacecraft.
International Space Station

The ISS also uses Whipple shielding to protect its interior from minor debris.[129] However, exterior portions (notably its solar panels) cannot be protected easily. In 1989, the ISS panels were predicted to degrade approximately 0.23% in four years due to the "sandblasting" effect of impacts with small orbital debris.[130] An avoidance maneuver is typically performed for the ISS if "there is a greater than one-in-10,000 chance of a debris strike".[131] As of January 2014, there have been sixteen maneuvers in the fifteen years the ISS had been in orbit.[131] By 2019, over 1,400 meteoroid and orbital debris (MMOD) impacts had been recorded on the ISS.[132]

As another method to reduce the risk to humans on board, ISS operational management asked the crew to shelter in the Soyuz on three occasions due to late debris-proximity warnings. In addition to the sixteen thruster firings and three Soyuz-capsule shelter orders, one attempted maneuver was not completed due to not having the several days' warning necessary to upload the maneuver timeline to the station's computer.[131][133][134] A March 2009 event involved debris believed to be a 10 cm (3.9 in) piece of the Kosmos 1275 satellite.[135] In 2013, the ISS operations management did not make a maneuver to avoid any debris, after making a record four debris maneuvers the previous year.[131]

Kessler syndrome

 
Growth of tracked objects in orbit and related events;[136] efforts to manage outer space global commons have so far not reduced the debris or the growth of objects in orbit

The Kessler syndrome,[137][138] proposed by NASA scientist Donald J. Kessler in 1978, is a theoretical scenario in which the density of objects in low Earth orbit (LEO) is high enough that collisions between objects could cause a cascade effect where each collision generates space debris that increases the likelihood of further collisions.[139] He further theorized that one implication, if this were to occur, is that the distribution of debris in orbit could render space activities and the use of satellites in specific orbital ranges economically impractical for many generations.[139]

The growth in the number of objects as a result of the late-1990s studies sparked debate in the space community on the nature of the problem and the earlier dire warnings. According to Kessler's 1991 derivation and 2001 updates,[140] the LEO environment in the 1,000 km (620 mi) altitude range should be cascading. However, only one major satellite collision incident occurred: the 2009 satellite collision between Iridium 33 and Cosmos 2251. The lack of obvious short-term cascading has led to speculation that the original estimates overstated the problem.[141] According to Kessler in 2010 however, a cascade may not be obvious until it is well advanced, which might take years.[142]

On Earth

 
Saudi officials inspect a crashed PAM-D module in January 2001.

Although most debris burns up in the atmosphere, larger debris objects can reach the ground intact. According to NASA, an average of one cataloged piece of debris has fallen back to Earth each day for the past 50 years. Despite their size, there has been no significant property damage from the debris.[143] Burning up in the atmosphere may also contribute to atmospheric pollution.[144] Numerous small cylindrical tanks from space objects have been found, designed to hold fuel or gasses.[145]

Tracking and measurement

Tracking from the ground

Radar and optical detectors such as lidar are the main tools for tracking space debris. Although objects under 10 cm (4 in) have reduced orbital stability, debris as small as 1 cm can be tracked,[146][147] however determining orbits to allow re-acquisition is difficult. Most debris remain unobserved. The NASA Orbital Debris Observatory tracked space debris with a 3 m (10 ft) liquid mirror transit telescope.[148] FM Radio waves can detect debris, after reflecting off them onto a receiver.[149] Optical tracking may be a useful early-warning system on spacecraft.[150]

The U.S. Strategic Command keeps a catalog of known orbital objects, using ground-based radar and telescopes, and a space-based telescope (originally to distinguish from hostile missiles). The 2009 edition listed about 19,000 objects.[151] Other data come from the ESA Space Debris Telescope, TIRA,[152] the Goldstone, Haystack,[153] and EISCAT radars and the Cobra Dane phased array radar,[154] to be used in debris-environment models like the ESA Meteoroid and Space Debris Terrestrial Environment Reference (MASTER).

Measurement in space

 
The Long Duration Exposure Facility (LDEF) is an important source of information on small-particle space debris.

Returned space hardware is a valuable source of information on the directional distribution and composition of the (sub-millimetre) debris flux. The LDEF satellite deployed by mission STS-41-C Challenger and retrieved by STS-32 Columbia spent 68 months in orbit to gather debris data. The EURECA satellite, deployed by STS-46 Atlantis in 1992 and retrieved by STS-57 Endeavour in 1993, was also used for debris study.[155]

The solar arrays of Hubble were returned by missions STS-61 Endeavour and STS-109 Columbia, and the impact craters studied by the ESA to validate its models. Materials returned from Mir were also studied, notably the Mir Environmental Effects Payload (which also tested materials intended for the ISS[156]).[157][158]

Gabbard diagrams

A debris cloud resulting from a single event is studied with scatter plots known as Gabbard diagrams, where the perigee and apogee of fragments are plotted with respect to their orbital period. Gabbard diagrams of the early debris cloud prior to the effects of perturbations, if the data were available, are reconstructed. They often include data on newly observed, as yet uncatalogued fragments. Gabbard diagrams can provide important insights into the features of the fragmentation, the direction and point of impact.[23][159]

Dealing with debris

An average of about one tracked object per day has been dropping out of orbit for the past 50 years,[160] averaging almost three objects per day at solar maximum (due to the heating and expansion of the Earth's atmosphere), but one about every three days at solar minimum, usually five and a half years later.[160] In addition to natural atmospheric effects, corporations, academics and government agencies have proposed plans and technology to deal with space debris, but as of November 2014, most of these are theoretical, and there is no extant business plan for debris reduction.[24]

A number of scholars have also observed that institutional factors—political, legal, economic, and cultural "rules of the game"—are the greatest impediment to the cleanup of near-Earth space. There is little commercial incentive to act, since costs are not assigned to polluters, though a number of technological solutions have been suggested.[24] However, effects to date are limited. In the US, governmental bodies have been accused of backsliding on previous commitments to limit debris growth, "let alone tackling the more complex issues of removing orbital debris."[161] The different methods for removal of space debris have been evaluated by the Space Generation Advisory Council, including French astrophysicist Fatoumata Kébé.[162]

Growth mitigation

 
Spatial density of LEO space debris by altitude, according to 2011 a NASA report to the United Nations Office for Outer Space Affairs[163]
 
Spatial density of space debris by altitude according to ESA MASTER-2001, without debris from the Chinese ASAT and 2009 collision events

As of the 2010s, several technical approaches to the mitigation of the growth of space debris are typically undertaken, yet no comprehensive legal regime or cost assignment structure is in place to reduce space debris in the way that terrestrial pollution has reduced since the mid-20th century.

To avoid excessive creation of artificial space debris, many—but not all—satellites launched to above-low-Earth-orbit are launched initially into elliptical orbits with perigees inside Earth's atmosphere so the orbit will quickly decay and the satellites then will destroy themselves upon reentry into the atmosphere. Other methods are used for spacecraft in higher orbits. These include passivation of the spacecraft at the end of its useful life; as well as the use of upper stages that can reignite to decelerate the stage to intentionally deorbit it, often on the first or second orbit following payload release; satellites that can, if they remain healthy for years, deorbit themselves from the lower orbits around Earth. Other satellites (such as many CubeSats) in low orbits below approximately 400 km (250 mi) orbital altitude depend on the energy-absorbing effects of the upper atmosphere to reliably deorbit a spacecraft within weeks or months.

Increasingly, spent upper stages in higher orbits—orbits for which low-delta-v deorbit is not possible, or not planned for—and architectures that support satellite passivation, at end of life are passivated at end of life. This removes any internal energy contained in the vehicle at the end of its mission or useful life. While this does not remove the debris of the now derelict rocket stage or satellite itself, it does substantially reduce the likelihood of the spacecraft destructing and creating many smaller pieces of space debris, a phenomenon that was common in many of the early generations of US and Soviet[71] spacecraft.

Upper stage passivation (e.g. of Delta boosters[28]) by releasing residual propellants reduces debris from orbital explosions; however even as late as 2011, not all upper stages implement this practice.[164] SpaceX used the term "propulsive passivation" for the final maneuver of their six-hour demonstration mission (STP-2) of the Falcon 9 second stage for the US Air Force in 2019, but did not define what all that term encompassed.[165]

With a "one-up, one-down" launch-license policy for Earth orbits, launchers would rendezvous with, capture and de-orbit a derelict satellite from approximately the same orbital plane.[166] Another possibility is the robotic refueling of satellites. Experiments have been flown by NASA,[167] and SpaceX is developing large-scale on-orbit propellant transfer technology.[168]

Another approach to debris mitigation is to explicitly design the mission architecture to always leave the rocket second-stage in an elliptical geocentric orbit with a low-perigee, thus ensuring rapid orbital decay and avoiding long-term orbital debris from spent rocket bodies. Such missions will often complete the payload placement in a final orbit by the use of low-thrust electric propulsion or with the use of a small kick stage to circularize the orbit. The kick stage itself may be designed with the excess-propellant capability to be able to self-deorbit.[169]

Self-removal

Although the ITU requires geostationary satellites to move to a graveyard orbit at the end of their lives, the selected orbital areas do not sufficiently protect GEO lanes from debris.[60] Rocket stages (or satellites) with enough propellant may make a direct, controlled de-orbit, or if this would require too much propellant, a satellite may be brought to an orbit where atmospheric drag would cause it to eventually de-orbit. This was done with the French Spot-1 satellite, reducing its atmospheric re-entry time from a projected 200 years to about 15 by lowering its altitude from 830 km (516 mi) to about 550 km (342 mi).[170][171]

The Iridium constellation – 95 communication satellites launched during the five-year period between 1997 and 2002 – provides a set of data points on the limits of self-removal. The satellite operator – Iridium Communications – remained operational over the two-decade life of the satellites (albeit with a company name change through a corporate bankruptcy during the period) and, by December 2019, had "completed disposal of the last of its 65 working legacy satellites."[172] However, this process left 30 satellites with a combined mass of (20,400 kg (45,000 lb), or nearly a third of the mass of this constellation) in LEO orbits at approximately 700 km (430 mi) altitude, where self-decay is quite slow. Of these satellites, 29 simply failed during their time in orbit and were thus unable to self-deorbit, while one – Iridium 33 – was involved in the 2009 satellite collision with the derelict Russian military satellite Kosmos-2251.[172] No contingency plan was laid for the removal of satellites that were unable to remove themselves. In 2019, the Iridium CEO, Matt Desch, said that Iridium would be willing to pay an active-debris-removal company to deorbit its remaining first-generation satellites if it were possible for an unrealistically low cost, say "US$10,000 per deorbit, but [he] acknowledged that price would likely be far below what a debris-removal company could realistically offer. 'You know at what point [it’s] a no-brainer, but [I] expect the cost is really in the millions or tens of millions, at which price I know it doesn’t make sense.'"[172]

Passive methods of increasing the orbital decay rate of spacecraft debris have been proposed. Instead of rockets, an electrodynamic tether could be attached to a spacecraft at launch; at the end of its lifetime, the tether would be rolled out to slow the spacecraft.[173] Other proposals include a booster stage with a sail-like attachment[174] and a large, thin, inflatable balloon envelope.[175]

In late December 2022, ESA successfully carried out a demonstration of a breaking sail-based satellite deorbiter, ADEO, which could be used by mitigation measures and is part of ESA's Zero Debris Initiative. Around one year earlier, China also tested a drag sail.[176][177]

External removal

A variety of approaches have been proposed, studied, or had ground subsystems built to use other spacecraft to remove existing space debris. A consensus of speakers at a meeting in Brussels in October 2012, organized by the Secure World Foundation (a U.S. think tank) and the French International Relations Institute,[178] reported that removal of the largest debris would be required to prevent the risk to spacecraft becoming unacceptable in the foreseeable future (without any addition to the inventory of dead spacecraft in LEO). To date in 2019, removal costs and legal questions about ownership and the authority to remove defunct satellites have stymied national or international action. Current space law retains ownership of all satellites with their original operators, even debris or spacecraft which are defunct or threaten active missions.

Multiple companies made plans in the late 2010s to conduct external removal on their satellites in mid-LEO orbits. For example, OneWeb planned to utilize onboard self-removal as "plan A" for satellite deorbiting at the end of life, but if a satellite were unable to remove itself within one year of end of life, OneWeb would implement "plan B" and dispatch a reusable (multi-transport mission) space tug to attach to the satellite at an already built-in capture target via a grappling fixture, to be towed to a lower orbit and released for re-entry.[179][180]

Remotely controlled vehicles

A well-studied solution uses a remotely controlled vehicle to rendezvous with, capture, and return debris to a central station.[181] One such system is Space Infrastructure Servicing, a commercially developed refueling depot and service spacecraft for communications satellites in geosynchronous orbit originally scheduled for a 2015 launch.[182] The SIS would be able to "push dead satellites into graveyard orbits."[183] The Advanced Common Evolved Stage family of upper stages is being designed with a high leftover-propellant margin (for derelict capture and de-orbit) and in-space refueling capability for the high delta-v required to de-orbit heavy objects from geosynchronous orbit.[166] A tug-like satellite to drag debris to a safe altitude for it to burn up in the atmosphere has been researched.[184] When debris is identified the satellite creates a difference in potential between the debris and itself, then using its thrusters to move itself and the debris to a safer orbit.

A variation of this approach is for the remotely controlled vehicle to rendezvous with debris, capture it temporarily to attach a smaller de-orbit satellite and drag the debris with a tether to the desired location. The "mothership" would then tow the debris-smallsat combination for atmospheric entry or move it to a graveyard orbit. One such system is the proposed Busek ORbital DEbris Remover (ORDER), which would carry over 40 SUL (satellite on umbilical line) de-orbit satellites and propellant sufficient for their removal.[24]

On 7 January 2010 Star, Inc. reported that it received a contract from the Space and Naval Warfare Systems Command for a feasibility study of the ElectroDynamic Debris Eliminator (EDDE) propellantless spacecraft for space-debris removal.[185] In February 2012 the Swiss Space Center at École Polytechnique Fédérale de Lausanne announced the Clean Space One project, a nanosatellite demonstration project for matching orbit with a defunct Swiss nanosatellite, capturing it and de-orbiting together.[186] The mission has seen several evolutions to reach a pac-man inspired capture model.[187] In 2013, Space Sweeper with Sling-Sat (4S), a grappling satellite which captures and ejects debris was studied.[188][needs update] In 2022, a Chinese satellite, SJ-21, grabbed an unused satellite and "threw" it into an orbit with a lower risk for it to collide.[189][190]

In December 2019, the European Space Agency awarded the first contract to clean up space debris. The €120 million mission dubbed ClearSpace-1 (a spinoff from the EPFL project) is slated to launch in 2025. It aims to remove a 100 kg VEga Secondary Payload Adapter (Vespa)[191] left by Vega flight VV02 in an 800 km (500 mi) orbit in 2013. A "chaser" will grab the junk with four robotic arms and drag it down to Earth's atmosphere where both will burn up.[192]

Laser methods

The laser broom uses a ground-based laser to ablate the front of the debris, producing a rocket-like thrust that slows the object. With continued application, the debris would fall enough to be influenced by atmospheric drag.[193][194] During the late 1990s, the U.S. Air Force's Project Orion was a laser-broom design.[195] Although a test-bed device was scheduled to launch on a Space Shuttle in 2003, international agreements banning powerful laser testing in orbit limited its use to measurements.[196] The 2003 Space Shuttle Columbia disaster postponed the project and according to Nicholas Johnson, chief scientist and program manager for NASA's Orbital Debris Program Office, "There are lots of little gotchas in the Orion final report. There's a reason why it's been sitting on the shelf for more than a decade."[197]

The momentum of the laser-beam photons could directly impart a thrust on the debris sufficient to move small debris into new orbits out of the way of working satellites. NASA research in 2011 indicates that firing a laser beam at a piece of space junk could impart an impulse of 1 mm (0.039 in) per second, and keeping the laser on the debris for a few hours per day could alter its course by 200 m (660 ft) per day.[198] One drawback is the potential for material degradation; the energy may break up the debris, adding to the problem.[199] A similar proposal places the laser on a satellite in Sun-synchronous orbit, using a pulsed beam to push satellites into lower orbits to accelerate their reentry.[24] A proposal to replace the laser with an Ion Beam Shepherd has been made,[200] and other proposals use a foamy ball of aerogel or a spray of water,[201] inflatable balloons,[202] electrodynamic tethers,[203] electroadhesion,[204] and dedicated anti-satellite weapons.[205]

Nets

On 28 February 2014, Japan's Japan Aerospace Exploration Agency (JAXA) launched a test "space net" satellite. The launch was an operational test only.[206] In December 2016 the country sent a space junk collector via Kounotori 6 to the ISS by which JAXA scientists experiment to pull junk out of orbit using a tether.[207][208] The system failed to extend a 700-meter tether from a space station resupply vehicle that was returning to Earth.[209][210] On 6 February the mission was declared a failure and leading researcher Koichi Inoue told reporters that they "believe the tether did not get released".[211]

Since 2012, the European Space Agency has been working on the design of a mission to remove large space debris from orbit. The mission, e.Deorbit, is scheduled for launch during 2023 with an objective to remove debris heavier than 4,000 kilograms (8,800 lb) from LEO.[212] Several capture techniques are being studied, including a net, a harpoon and a combination robot arm and clamping mechanism.[213]

Harpoon

The RemoveDEBRIS mission plan is to test the efficacy of several ADR technologies on mock targets in low Earth orbit. In order to complete its planned experiments the platform is equipped with a net, a harpoon, a laser ranging instrument, a dragsail, and two CubeSats (miniature research satellites).[214] The mission was launched on 2 April 2018.

National and international regulation

There is no international treaty minimizing space debris. However, the United Nations Committee on the Peaceful Uses of Outer Space (COPUOS) published voluntary guidelines in 2007,[215] using a variety of earlier national regulatory attempts at developing standards for debris mitigation. As of 2008, the committee was discussing international "rules of the road" to prevent collisions between satellites.[216] By 2013, a number of national legal regimes existed,[217][218][219] typically instantiated in the launch licenses that are required for a launch in all spacefaring nations.[220]

The U.S. issued a set of standard practices for civilian (NASA) and military (DoD and USAF) orbital-debris mitigation in 2001.[221][222][218] The standard envisioned disposal for final mission orbits in one of three ways: 1) atmospheric reentry where even with "conservative projections for solar activity, atmospheric drag will limit the lifetime to no longer than 25 years after completion of mission;" 2) maneuver to a "storage orbit:" move the spacecraft to one of four very broad parking orbit ranges (2,000–19,700 km (1,200–12,200 mi), 20,700–35,300 km (12,900–21,900 mi), above 36,100 km (22,400 mi), or out of Earth orbit completely and into any heliocentric orbit; 3) "Direct retrieval: Retrieve the structure and remove it from orbit as soon as practicable after completion of mission."[217] The standard articulated in option 1, which is the standard applicable to most satellites and derelict upper stages launched, has come to be known as the "25-year rule."[223] The US updated the Orbital Debris Mitigation Standard Practices (ODMSP) in December 2019, but made no change to the 25-year rule even though "[m]any in the space community believe that the timeframe should be less than 25 years."[224] There is no consensus however on what any new timeframe might be.[224]

In 2002, the European Space Agency (ESA) worked with an international group to promulgate a similar set of standards, also with a "25-year rule" applying to most Earth-orbit satellites and upper stages. Space agencies in Europe began to develop technical guidelines in the mid-1990s, and ASI, UKSA, CNES, DLR and ESA signed a "European Code of Conduct" in 2006,[219] which was a predecessor standard to the ISO international standard work that would begin the following year. In 2008, ESA further developed "its own "Requirements on Space Debris Mitigation for Agency Projects" which "came into force on 1 April 2008."[219]

Germany and France have posted bonds to safeguard the property from debris damage.[clarification needed][225] The "direct retrieval" option (option no. 3 in the US "standard practices" above) has rarely been done by any spacefaring nation (exception, USAF X-37) or commercial actor since the earliest days of spaceflight due to the cost and complexity of achieving direct retrieval, but the ESA has scheduled a 2025 demonstration mission (Clearspace-1) to do this with a single small 100 kg (220 lb) derelict upper stage at a projected cost of €120 million not including the launch costs.[192]

By 2006, the Indian Space Research Organization (ISRO) had developed a number of technical means of debris mitigation (upper stage passivation, propellant reserves for movement to graveyard orbits, etc.) for ISRO launch vehicles and satellites, and was actively contributing to inter-agency debris coordination and the efforts of the UN COPUOS committee.[226]

In 2007, the ISO began preparing an international standard for space-debris mitigation.[227] By 2010, ISO had published "a comprehensive set of space system engineering standards aimed at mitigating space debris. [with primary requirements] defined in the top-level standard, ISO 24113." By 2017, the standards were nearly complete. However, these standards are not binding on any party by ISO or any international jurisdiction. They are simply available for use in any of a variety of voluntary ways. They "can be adopted voluntarily by a spacecraft manufacturer or operator, or brought into effect through a commercial contract between a customer and supplier, or used as the basis for establishing a set of national regulations on space debris mitigation."[223]

The voluntary ISO standard also adopted the "25-year rule" for the "LEO protected region" below 2,000 km (1,200 mi) altitude that has been previously (and still is, as of 2019) used by the US, ESA, and UN mitigation standards, and identifies it as "an upper limit for the amount of time that a space system shall remain in orbit after its mission is completed. Ideally, the time to deorbit should be as short as possible (i.e., much shorter than 25 years)".[223]

Holger Krag of the European Space Agency states that as of 2017 there is no binding international regulatory framework with no progress occurring at the respective UN body in Vienna.[105]

Barriers

With the rapid development of the computer and digitalization industries, more countries and companies have engaged in space activities since the turn of the 20th century. The tragedy of the commons is an economic theory referring to a situation where maximizing self-interest through using a shared resource can finally lead to the resource degradation shared by all.[228] Based on the theory, individuals’ rational action in space will finally lead to an irrational collective result: orbits are crowded with debris. As a common-pool resource, the Earth's orbits, especially LEO and GEO that accommodate most satellites, are nonexcludable and rivalry.[229] To address the tragedy and ensure space sustainability, many technical approaches have been developed. And in terms of governance mechanisms, the top-down centralized one is less suitable to tackle the complex debris problem due to the increasing number of space actors.[230] Instead, much evidence has proved that polycentric form of governance developed by Elinor Ostrom can work in space.[231]

In the process of promoting the polycentric network, there are some existing barriers needed to be dealt with.

Incomplete data of space debris

As orbital debris is a global problem affecting both spacefaring and non-spacefaring nations, it is necessary to be handled in a worldwide context.[228] Because of the complexity and dynamics of object movements like spacecrafts, debris, meteorites, etc., many countries and regions including the United States, Europe, Russia and China have developed their space situational awareness (SSA) to avoid potential threats in space or plan actions in advance.[232] To a certain extent, SSA plays a role in tracking space debris. In order to build a powerful SSA system, there are two prerequisites: international cooperation and exchange of information and data.[232] However, limitations still exist in spite of the substantially improving data quality over the past decades. Some space powers are not willing to share the information that they have collected, and those, such as the U.S., that have shared the data keep parts of it secret.[233] Instead of joining in a coordinated way, a great deal of SSA programs and national databases run parallel to each other with some overlaps, hindering the formation of a collaborative monitoring system.[233]

Some private actors are also trying to establish SSA systems. For example, the Space Data Association (SDA) formed in 2009 is a non-governmental entity. It currently consists of 21 global satellite operators and 4 executive members: Eutelsat, Inmarsat, Intelsat and SES. SDA is a non-profit platform, aiming to avoid radio interference and space collisions through pooling data from operators independently.[232] Researchers suggest that it is essential to establish an international center for exchanging information on space debris because SSA networks do not completely equal debris tracking systems — the former ones focus more on active and threatening objects in space.[234] And in terms of debris populations and defunct satellites, not very much operators have provided data.[234]

In a polycentric governance network, a resource that cannot be holistically monitored is less possible to be well managed.[233] Both insufficient transnational cooperation and information sharing bring resistance to addressing the debris problem. There is still a long way to go before building a global network that covers complete data and has strong interconnection and interoperability.

Insufficient participation of private actors

With the commercialization of satellites and space, the private sector is getting more interested in space activities. For example, SpaceX is planning to create a network of around 12,000 small satellites that can transmit high-speed internet to any place in the world.[235] The proportion of commercial spacecrafts has increased from 4.6% in the 1980s to 55.6% in the 2010s.[236] Despite the high participation rate of commercial entities, UN COPUOS once deliberately excluded them from having a voice in discussions unless being formally invited by a member state.[230] Ostrom said that the involvement of all relevant stakeholders in the rule-design and implementation process is one of the critical elements of successful governance.[237] The exclusion of private actors largely reduces the effectiveness of the committee's role in making collective-choice arrangements that reflect the interests of all space users.[230]

The limited engagement of private actors slows down the process of addressing space debris to some degree.[238] Ties existing between dissimilar stakeholders in the governance network offer access to diverse resources.[239] Different competence among stakeholders can help allocate the tasks more reasonably. In that case, the expertise and experience of private operators are critical to help the world achieve space sustainability.[238] The complementary strengths of different stakeholders enable the governance network to be more adaptable to changes and reach common goals more effectively.[239] In recent years, many private actors have seen commercial opportunities of eliminating space debris. It is estimated that by 2022 the global market for debris monitoring and removal will generate a revenue of around $2.9 billion.[240] For example, Astroscale has contracted with European and Japanese space agencies to develop the capacity of removing orbital debris.[241] Despite that, they are still in small quantity compared to the number of those who have placed satellites in space. Privateer Space, a Hawaiian-based startup company started by American engineer Alex Fielding, space environmentalist Dr. Moriba Jah, and Apple co-founder Steve Wozniak, announced plans in September 2021 to launch hundreds of satellites into orbit in order to study space debris.[242] However, the company stated it is in "stealth mode" and no such satellites have been launched.[242]

Fortunately, the current space exploration is not completely driven by competition, and there still exists a chance for dialogues and cooperation among all stakeholders in both developed and developing countries, to reach an agreement on tackling space debris and assure an equitable and orderly exploration.[243] Besides private actors, network governance does not necessarily exclude the states from playing a role. Instead, the different functions of states might promote the governance process.[244] To improve the polycentric governance network of space debris, researchers suggest: encourage data-sharing among different national and organizational databases at the political level; develop shared standards for data collection systems to improve interoperability; enhance the participation of private actors through involving them in national and international discussions.[233]

Environmental concerns

The continued practice of disposing of space debris on Earth in areas such as the spacecraft cemetery has raised environmental concerns.[245] Klinger states that "the environmental geopolitics of Earth and outer space are inextricably linked by the spatial politics of privilege and sacrifice – among people, places, and institutions".[245][246] Since 1971, 273 spacecraft and satellites have been directed to Point Nemo; this number includes the Mir Space Station (142 tonnes) and will include the International Space Station in 2024 (240 tonnes). In 2018, it was found that the water had 26 microplastic particles per cubic metre, meaning it is highly polluted.[247] The prevalence of orbital debris has been likened to the terrestrial environmental phenomenon of "sacrifice zones," which are designated geographic regions with high levels of environmental degradation.

Since the 1960s, over three hundred rocket launch sites have been built globally.[245] Among these launch sites, 17 hosted 90 launches in 2017 alone.[245] Rocket launches affect local and global environments through the construction of necessary infrastructure, exposure of local environments to toxic residue and the dispersal of pollutants.[245] Rockets are the only source of direct anthropogenic emissions into the stratosphere and emit ozone depleting substances such as nitrous oxide, hydrogen chloride and aluminium oxide; these substances can destroy 105 ozone molecules before depleting.[245] Each launch showers an area concentrated within a kilometre with toxins, heavy metals, and acids.[245] This results in localised regional acid rain, plant death, fish kills, and failed seed germination.[245] Furthermore, studies on trace elements concentration in alligators, near NASA launch activities in Florida (USA), showed that over 50% of alligators had "greater than toxic levels" of trace elements in their liver.[245] Similarly, research in Kazakhstan, Russia and China has found that unsymmetrical dimethylhydrazine (UDMH) has carcinogenic, mutagenic, convulsant, teratogenic, embryotoxic and DNA damaging effects on rodents living near the Baikonur Cosmodrome, Kazakhstan.[248] It is unknown, however, at what trace concentrations these toxic effects manifest in humans or how it may bioaccumulate up the food chain.[248] A lack of adequate resourcing to maintain safe, non-toxic environments makes these areas sacrifice zones and spaces of waste. The relative remoteness of these spaces makes them attractive launch sites, yet this "periphery" remain central to both their human and non-human inhabitants, who become "sacrificial".[249][250][245]

Orbital debris as a question of environmental justice

An increase in anthropogenic activity in outer space has resulted in large amounts of physical pollution known as orbital debris.[251] This has resulted in space becoming more and more congested due to this rapid increase.[252] This increase in congestion threatens the orbital operations of nations and corporations alike.[251] However, orbital debris also has an impact on the wider population through various means, such as potentially lethal debris falling from the sky,[253] or orbital debris ruining night skies through light pollution.[254] Environmental justice as described by the United States Environmental Protection Agency is the fair and meaningful involvement of all demographics in the development and implementation of environmental regulations and policies.[255] Outer space can be seen as an environment like any other environment on Earth,[256] making orbital debris a potential issue of environmental justice.

The idea of environmental injustice is also that the rights of those who have suffered environmental harm or have been disrupted and encroached upon by more powerful actors are protected.[256] In the context of the space industry large space organisations and nations are the powerful actors and those who have suffered are public. Recent research shows that space exploration opens many questions about environmental justice.[257] Environmental geopolitics of the earth and that of outer space are linked, particularly by the geopolitics of privilege from one party and sacrifice from another.[256] They are also linked in the premise of environmental justice, this injustice can unfold on multiple scales such as emission from space launches, placement of outer space-related infrastructure and of course orbital debris in this case.[256]

There is an argument that as well as viewing space as an environment space should also be viewed as a commons.[258] If space is viewed as a commons then its resources need to be managed for the common good of all people. If not, then this poses a risk of injustice. By managing space as a resource that all nations have access to, and none can claim sovereignity over, outer space can be also understood as an example of a global commons. However, legally defining space as a common is challenging, as the idea of global commons is a social construct.[252] Many space treaties include various phrases describing and defining the usage of outer space, including phrases such as "for the benefit of all people" and "shall be the providence of all mankind".[259] However, none of these treaties provides an adequate framework for handling resources or resolving issues.[259]

Governance frameworks for outer space have a very narrow and utilitarian view of outer space that looks at what they can gain from exploration.[260]

At other celestial bodies

 
A piece of a thermal blanket that may have come from the descent stage of the Perseverance
 
Perseverance's backshell sitting upright on the surface of Jezero Crater

The issue of space debris has been raised as a mitigation challenge for missions around the Moon with the danger of increasing space debris around it.[261][262]

In 2022, several elements of space debris were found on Mars, Perseverance's backshell was found on the surface of Jezero Crater,[263] and a piece of a thermal blanket that may have come from the descent stage of the rover.[264][265]

It is thought that on 4 March 2022, for the first time, human space debris – most likely a spent rocket body, Long March 3C third stage from the 2014 Chang'e 5 T1 mission – unintentionally hit the lunar surface, creating an unexpected double crater.[266][267]

In popular culture

Until the End of the World (1991) is a French sci-fi drama set under the backdrop of an out-of-control Indian nuclear satellite, predicted to re-enter the atmosphere, threatening vast populated areas of the Earth.[268]

Gravity, a 2013 survival film directed by Alfonso Cuaron, is about a disaster on a space mission caused by Kessler syndrome.[269]

In season 1 of Love, Death & Robots (2019), episode 11, "Helping Hand", revolves around an astronaut being struck by a screw from space debris which knocks her off a satellite in orbit.[270]

Manga and anime Planetes tells a story about a crew of Space Debris station that collects and disposes space debris.[271]

See also

References

Citations

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Bibliography

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  • Hoots, Felix; Schumacher, Paul Jr.; Glover, Robert A. (2004). "History of Analytical Orbit Modeling in the U.S. Space Surveillance System". Journal of Guidance, Control, and Dynamics. 27 (2): 174–185. Bibcode:2004JGCD...27..174H. doi:10.2514/1.9161.
  • Johnson, Nicholas L. (1998). "Monitoring and Controlling Debris in Space". Scientific American. 279 (2): 62–67. Bibcode:1998SciAm.279b..62J. doi:10.1038/scientificamerican0898-62. JSTOR 26070599. Retrieved 21 January 2023..
  • Kessler, Donald (1971). "Estimate of Particle Densities and Collision Danger for Spacecraft Moving Through the Asteroid Belt". Physical Studies of Minor Planets. NASA SP-267. 267: 595–605. Bibcode:1971NASSP.267..595K..
  • Kessler, Donald; Cour-Palais, Burton (June 1978). (PDF). Journal of Geophysical Research. 81 (A6): 2637–46. Bibcode:1978JGR....83.2637K. doi:10.1029/JA083iA06p02637. Archived from the original (PDF) on 15 May 2011..
  • Kessler, Donald (1981). (PDF). Journal of Spacecraft. 16 (4): 357–60. Bibcode:1981JSpRo..18..357K. doi:10.2514/3.57828. Archived from the original (PDF) on 14 July 2010..
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Further reading

  • , Center for Orbital and Reentry Debris Studies, Aerospace Corporation
  • Committee for the Assessment of NASA's Orbital Debris Programs (2011). Limiting Future Collision Risk to Spacecraft: An Assessment of NASA's Meteoroid and Orbital Debris Programs. Washington, D.C.: National Research Council. ISBN 978-0-309-21974-7.
    • Klotz, Irene (1 September 2011). "Space junk reaching 'tipping point,' report warns". Reuters. Retrieved 2 September 2011. News item summarizing the above report
  • Steven A. Hildreth and Allison Arnold. Threats to U.S. National Security Interests in Space: Orbital Debris Mitigation and Removal. Washington, D.C.: Congressional Research Service, 8 January 2014.
  • David Leonard, "The Clutter Above", Bulletin of the Atomic Scientists, July/August 2005.
  • Patrick McDaniel, "A Methodology for Estimating the Uncertainty in the Predicted Annual Risk to Orbiting Spacecraft from Current or Predicted Space Debris Population". National Defense University, 1997.
  • "Interagency Report on Orbital Debris, 1995", National Science and Technology Council, November 1995.
  • Nickolay Smirnov, Space Debris: Hazard Evaluation and Mitigation. Boca Raton, FL: CRC Press, 2002, ISBN 0-415-27907-0.
  • Richard Talcott, "How We Junked Up Outer Space", Astronomy, Volume 36, Issue 6 (June 2008), pp. 40–43.
  • "Technical report on space debris, 1999", United Nations, 2006. ISBN 92-1-100813-1.
  • Robin Biesbroek (2015). Active Debris Removal in Space: How to Clean the Earth's Environment from Space Debris. CreateSpace. ISBN 978-1-5085-2918-7.
  • Khatchadourian, Raffi, "The Trash Nebula: Millions of man-made artifacts are circling Earth. Will one of them cause a disaster?", 28 September 2020, pp. 44–52, 54–55. "By one estimate, there are a hundred million bits of debris that are a millimetre in size, a hundred million as small as a micron. We live in a corona of trash. [T]he problem, if ignored, could destroy all the satellites that orbit near the Earth – a loss that would be more acutely felt as humanity increasingly relied on space." (p. 47.)

External links

  • Sativew – Tracking Space Junk in real time
  • NASA Orbital Debris Program Office
  • ESA Space Debris Office 5 September 2012 at the Wayback Machine
  • , documentary film
  • EISCAT Space Debris during the international polar year
  • Intro to mathematical modeling of space debris flux 28 February 2019 at the Wayback Machine
  • SOCRATES: A free daily service predicting close encounters on orbit between satellites and debris orbiting Earth
  • A summary of current space debris by type and orbit
  • Space Junk Astronomy Cast episode No. 82, includes full transcript
  • Space Debris Illustrated: The Problem in Pictures
  • PACA: Space Debris
  • The Threat of Orbital Debris and Protecting NASA Space Assets from Satellite Collisions
  • Space Age Wasteland: Debris in Orbit Is Here to Stay; Scientific American; 2012
  • United States Space Surveillance Network
  • PATENDER: GMV’S Trailblazing low-gravity space-debris capture system
  • Space Junk Infographic
  • Stuff In Space
  • Astria Graph

space, debris, space, junk, redirects, here, other, uses, space, junk, disambiguation, cosmic, debris, redirects, here, frank, zappa, song, cosmik, debris, also, known, space, junk, space, pollution, space, waste, space, trash, space, garbage, cosmic, debris, . Space Junk redirects here For other uses see Space Junk disambiguation Cosmic debris redirects here For the Frank Zappa song see Cosmik Debris Space debris also known as space junk space pollution 1 space waste space trash space garbage or cosmic debris 2 are defunct human made objects in space principally in Earth orbit which no longer serve a useful function These include derelict spacecraft nonfunctional spacecraft and abandoned launch vehicle stages mission related debris and particularly numerous in Earth orbit fragmentation debris from the breakup of derelict rocket bodies and spacecraft In addition to derelict human made objects left in orbit other examples of space debris include fragments from their disintegration erosion and collisions or even paint flecks solidified liquids expelled from spacecraft and unburned particles from solid rocket motors Space debris represents a risk to spacecraft 3 A computer generated image representing the locations but not relative sizes of space debris as could be seen from high Earth orbit The two main debris fields are the ring of objects in geosynchronous Earth orbit GEO and the cloud of objects in low Earth orbit LEO Space debris is typically a negative externality it creates an external cost on others from the initial action to launch or use a spacecraft in near Earth orbit a cost that is typically not taken into account nor fully accounted for in the cost 4 5 by the launcher or payload owner 6 1 7 Several spacecraft both crewed and uncrewed have been damaged or destroyed by space debris The measurement mitigation and potential removal of debris are conducted by some participants in the space industry 8 As of November 2022 update the US Space Surveillance Network reported 25 857 artificial objects in orbit above the Earth 9 including 5 465 operational satellites 10 However these are just the objects large enough to be tracked and in an orbit that makes tracking possible Satellite debris that is in a Molnya orbit such as the Kosmos Ono series might be too high above the northern hemisphere to be tracked 11 As of January 2019 update more than 128 million pieces of debris smaller than 1 cm 0 4 in about 900 000 pieces of debris 1 10 cm and around 34 000 of pieces larger than 10 cm 3 9 in were estimated to be in orbit around the Earth 8 When the smallest objects of artificial space debris paint flecks solid rocket exhaust particles etc are grouped with micrometeoroids they are together sometimes referred to by space agencies as MMOD Micrometeoroid and Orbital Debris Collisions with debris have become a hazard to spacecraft the smallest objects cause damage akin to sandblasting especially to solar panels and optics like telescopes or star trackers that cannot easily be protected by a ballistic shield 12 Below 2 000 km 1 200 mi Earth altitude pieces of debris are denser than meteoroids most are dust from solid rocket motors surface erosion debris like paint flakes and frozen coolant from Soviet nuclear powered satellites 13 14 15 For comparison the International Space Station orbits in the 300 400 kilometres 190 250 mi range while the two most recent large debris events the 2007 Chinese antisat weapon test and the 2009 satellite collision occurred at 800 to 900 kilometres 500 to 560 mi altitude 16 The ISS has Whipple shielding to resist damage from small MMOD however known debris with a collision chance over 1 10 000 are avoided by maneuvering the station Contents 1 History 1 1 Debris growth 1 1 1 Debris history in particular years 2 Characterization 2 1 Size 2 2 Low Earth orbit 2 3 Higher altitudes 3 Sources 3 1 Dead spacecraft 3 2 Lost equipment 3 3 Boosters 3 4 Weapons 4 Hazards 4 1 To spacecraft 4 1 1 Uncrewed spacecraft 4 1 2 Crewed spacecraft 4 1 2 1 Space Shuttle missions 4 1 2 2 Mir 4 1 2 3 International Space Station 4 1 3 Kessler syndrome 4 2 On Earth 5 Tracking and measurement 5 1 Tracking from the ground 5 2 Measurement in space 5 3 Gabbard diagrams 6 Dealing with debris 6 1 Growth mitigation 6 2 Self removal 6 3 External removal 6 3 1 Remotely controlled vehicles 6 3 2 Laser methods 6 3 3 Nets 6 3 4 Harpoon 6 4 National and international regulation 6 5 Barriers 6 5 1 Incomplete data of space debris 6 5 2 Insufficient participation of private actors 6 6 Environmental concerns 6 6 1 Orbital debris as a question of environmental justice 7 At other celestial bodies 8 In popular culture 9 See also 10 References 10 1 Citations 10 2 Bibliography 11 Further reading 12 External linksHistory EditSpace debris began to accumulate in Earth orbit immediately with the first launch of an artificial satellite Sputnik 1 into orbit in October 1957 But even before that humans might have produced ejecta that became space debris as in the August 1957 Pascal B test 17 18 Going back even earlier there was natural ejecta from Earth in orbit After the launch of Sputnik the North American Aerospace Defense Command NORAD began compiling a database the Space Object Catalog of all known rocket launches and objects reaching orbit satellites protective shields and upper stages of launch vehicles NASA later published modified versions of the database in two line element set 19 and beginning in the early 1980s the CelesTrak bulletin board system re published them 20 Gabbard diagram of almost 300 pieces of debris from the disintegration of the five month old third stage of the Chinese Long March 4 booster on 11 March 2000 The trackers NORAD who fed the database were aware of other objects in orbit many of which were the result of in orbit explosions 21 Some were deliberately caused during the 1960s anti satellite weapon ASAT testing and others were the result of rocket stages blowing up in orbit as leftover propellant expanded and ruptured their tanks To improve tracking NORAD employee John Gabbard kept a more detailed database of as many objects as he could identify 22 Studying the explosions In March 1971 Gabbard developed a technique for predicting the orbital paths of their products and Gabbard diagrams or plots are now widely used These studies were used to improve the modeling of orbital evolution and decay 23 When the NORAD database became publicly available during the 1970s clarification needed techniques developed for the asteroid belt were applied to the study by whom to the database of known artificial satellite Earth objects citation needed Baker Nunn cameras were widely used to study space debris In addition to approaches to debris reduction where time and natural gravitational atmospheric effects help to clear space debris or a variety of technological approaches that have been proposed with most not implemented to reduce space debris a number of scholars have observed that institutional factors political legal economic and cultural rules of the game are the greatest impediment to the cleanup of near Earth space By 2014 there was little commercial incentive to reduce space debris since the cost of dealing with it is not assigned to the entity producing it but rather falls on all users of the space environment and rely on human society as a whole that benefits from space technologies and knowledge A number of suggestions for improving institutions so as to increase the incentives to reduce space debris have been made These include government mandates to create incentives as well as companies coming to see economic benefit to reducing debris more aggressively than existing government standard practices 24 In 1979 NASA founded the Orbital Debris Program to research mitigation measures for space debris in Earth orbit 25 26 Debris growth Edit During the 1980s NASA and other U S groups attempted to limit the growth of debris One trial solution was implemented by McDonnell Douglas in 1981 for the Delta launch vehicle by having the booster move away from its payload and vent any propellant remaining in its tanks 27 This eliminated one source for pressure buildup in the tanks which had previously caused them to explode and create additional orbital debris 28 Other countries were slower to adopt this measure and due especially to a number of launches by the Soviet Union the problem grew throughout the decade 29 A new battery of studies followed as NASA NORAD and others attempted to better understand the orbital environment with each adjusting the number of pieces of debris in the critical mass zone upward Although in 1981 when Schefter s article was published the number of objects was estimated at 5 000 21 new detectors in the Ground based Electro Optical Deep Space Surveillance system found new objects By the late 1990s it was thought that most of the 28 000 launched objects had already decayed and about 8 500 remained in orbit 30 By 2005 this was adjusted upward to 13 000 objects 31 and a 2006 study increased the number to 19 000 as a result of an ASAT and a satellite collision 32 In 2011 NASA said that 22 000 objects were being tracked 33 A 2006 NASA model suggested that if no new launches took place the environment would retain the then known population until about 2055 when it would increase on its own 34 35 Richard Crowther of Britain s Defence Evaluation and Research Agency said in 2002 that he believed the cascade would begin about 2015 36 The National Academy of Sciences summarizing the professional view noted widespread agreement that two bands of LEO space 900 to 1 000 km 620 mi and 1 500 km 930 mi were already past critical density 37 In the 2009 European Air and Space Conference University of Southampton researcher Hugh Lewis predicted that the threat from space debris would rise 50 percent in the next decade and quadruple in the next 50 years As of 2009 update more than 13 000 close calls were tracked weekly 38 A 2011 report by the U S National Research Council warned NASA that the amount of orbiting space debris was at a critical level According to some computer models the amount of space debris has reached a tipping point with enough currently in orbit to continually collide and create even more debris raising the risk of spacecraft failures The report called for international regulations limiting debris and research of disposal methods 39 Objects in Earth orbit including fragmentation debris November 2020 NASA ODPO Debris history in particular years Edit By mid 1994 there had been 68 breakups or debris anomalous events involving satellites launched by the former Soviet Union Russia and 18 similar events had been discovered involving rocket bodies and other propulsion related operational debris 40 As of 2009 update 19 000 debris over 5 cm 2 in were tracked by United States Space Surveillance Network 16 As of July 2013 update estimates of more than 170 million debris smaller than 1 cm 0 4 in about 670 000 debris 1 10 cm and approximately 29 000 larger pieces of debris are in orbit 41 As of July 2016 update nearly 18 000 artificial objects are orbiting above Earth 42 including 1 419 operational satellites 43 As of October 2019 update nearly 20 000 artificial objects in orbit above the Earth 9 including 2 218 operational satellites 10 Characterization EditSize Edit There are estimated to be over 128 million pieces of debris smaller than 1 cm 0 39 in as of January 2019 There are approximately 900 000 pieces from 1 to 10 cm The current count of large debris defined as 10 cm across or larger 44 is 34 000 8 The technical measurement cutoff clarification needed is c 3 mm 0 12 in 45 As of 2020 there are 8 000 metric tons of debris in orbit a figure that is expected to increase 46 Low Earth orbit Edit Satellite hit by a space debris animation by ESA In the orbits nearest to Earth less than 2 000 km 1 200 mi orbital altitude referred to as low Earth orbit LEO there have traditionally been few universal orbits that keep a number of spacecraft in particular rings in contrast to GEO a single orbit that is widely used by over 500 satellites This is beginning to change in 2019 and several companies have begun to deploy the early phases of satellite internet constellations which will have many universal orbits in LEO with 30 to 50 satellites per orbital plane and altitude Traditionally the most populated LEO orbits have been a number of sun synchronous satellites that keep a constant angle between the Sun and the orbital plane making Earth observation easier with consistent sun angle and lighting Sun synchronous orbits are polar meaning they cross over the polar regions LEO satellites orbit in many planes typically up to 15 times a day causing frequent approaches between objects The density of satellites both active and derelict is much higher in LEO 47 Orbits are affected by gravitational perturbations which in LEO include unevenness of the Earth s gravitational field due to variations in the density of the planet and collisions can occur from any direction The average impact speed of collisions in Low Earth Orbit is 10 km s with maximums reaching above 14 km s due to orbital eccentricity 48 The 2009 satellite collision occurred at a closing speed of 11 7 km s 26 000 mph 49 creating over 2 000 large debris fragments 50 These debris cross many other orbits and increase debris collision risk It is theorized that a sufficiently large collision of spacecraft could potentially lead to a cascade effect or even make some particular low Earth orbits effectively unusable for long term use by orbiting satellites a phenomenon known as the Kessler syndrome 51 The theoretical effect is projected to be a theoretical runaway chain reaction of collisions that could occur exponentially increasing the number and density of space debris in low Earth orbit and has been hypothesized to ensue beyond some critical density 52 Crewed space missions are mostly at 400 km 250 mi altitude and below where air drag helps clear zones of fragments The upper atmosphere is not a fixed density at any particular orbital altitude it varies as a result of atmospheric tides and expands or contracts over longer time periods as a result of space weather 53 These longer term effects can increase drag at lower altitudes the 1990s expansion was a factor in reduced debris density 54 Another factor was fewer launches by Russia the Soviet Union made most of their launches in the 1970s and 1980s 55 7 Higher altitudes Edit At higher altitudes where air drag is less significant orbital decay takes longer Slight atmospheric drag lunar perturbations Earth s gravity perturbations solar wind and solar radiation pressure can gradually bring debris down to lower altitudes where it decays but at very high altitudes this may take centuries 56 Although high altitude orbits are less commonly used than LEO and the onset of the problem is slower the numbers progress toward the critical threshold more quickly contradictory page needed 57 Many communications satellites are in geostationary orbits GEO clustering over specific targets and sharing the same orbital path Although velocities are low between GEO objects when a satellite becomes derelict such as Telstar 401 it assumes a geosynchronous orbit its orbital inclination increases about 8 and its speed increases about 160 km h 99 mph per year Impact velocity peaks at about 1 5 km s 0 93 mi s Orbital perturbations cause longitude drift of the inoperable spacecraft and precession of the orbital plane Close approaches within 50 meters are estimated at one per year 58 The collision debris pose less short term risk than from an LEO collision but the satellite would likely become inoperable Large objects such as solar power satellites are especially vulnerable to collisions 59 Although the ITU now requires proof a satellite can be moved out of its orbital slot at the end of its lifespan studies suggest this is insufficient 60 Since GEO orbit is too distant to accurately measure objects under 1 m 3 ft 3 in the nature of the problem is not well known 61 Satellites could be moved to empty spots in GEO requiring less maneuvering and making it easier to predict future motion 62 Satellites or boosters in other orbits especially stranded in geostationary transfer orbit are an additional concern due to their typically high crossing velocity Despite efforts to reduce risk spacecraft collisions have occurred The European Space Agency telecom satellite Olympus 1 was struck by a meteoroid on 11 August 1993 and eventually moved to a graveyard orbit 63 On 29 March 2006 the Russian Express AM11 communications satellite was struck by an unknown object and rendered inoperable 64 its engineers had enough contact time with the satellite to send it into a graveyard orbit Sources EditDead spacecraft Edit Main category Derelict satellites orbiting Earth Main category Spacecraft that broke apart in space Vanguard 1 is expected to remain in orbit for 240 years 65 66 In 1958 the United States launched Vanguard I into a medium Earth orbit MEO As of October 2009 update it the upper stage of its launch rocket and associated piece of debris are the oldest surviving artificial space objects still in orbit and are expected to be until after the year 2250 67 68 As of May 2022 update the Union of Concerned Scientists listed 5 465 operational satellites from a known population of 27 000 pieces of orbital debris tracked by NORAD 69 70 While sometimes satellites are simply left in orbit when they re no longer useful many countries require that satellites go through passivation at the end of their life They are then either boosted into a higher graveyard orbit or a lower short term orbit But even satellites that have been properly moved to a higher orbit have an eight percent probability of puncture and coolant release over a 50 year period The coolant freezes into droplets of solid sodium potassium alloy creating more debris 13 71 Despite the use of passivization or prior to its standardization many satellites and rocket bodies have exploded or broken apart on orbit In February 2015 for example the USAF Defense Meteorological Satellite Program Flight 13 DMSP F13 exploded on orbit creating at least 149 debris objects which were expected to remain in orbit for decades 72 Later that same year NOAA 16 which had been decommissioned after an anomaly in June 2014 broke apart on orbit into at least 275 pieces 73 For older programs such as the Soviet era Meteor 2 and Kosmos satellites design flaws resulted in numerous break ups at least 68 by 1994 following decommissioning resulting in more debris 40 In addition to the accidental creation of debris some has been made intentionally through the deliberate destruction of satellites This has been done as a test of anti satellite or anti ballistic missile technology or to prevent a sensitive satellite from being examined by a foreign power 40 The United States has conducted over 30 anti satellite weapons tests ASATs the Soviet Union Russia has performed at least 27 China has performed 10 and India has performed at least one 74 75 The most recent ASATs were the Chinese interception of FY 1C Russian trials of its PL 19 Nudol the American interception of USA 193 and India s interception of an unstated live satellite 75 Lost equipment Edit A drifting thermal blanket photographed in 1998 during STS 88 Space debris includes a glove lost by astronaut Ed White on the first American space walk EVA a camera lost by Michael Collins near Gemini 10 a thermal blanket lost during STS 88 garbage bags jettisoned by Soviet cosmonauts during Mir s 15 year life 76 a wrench and a toothbrush 77 Sunita Williams of STS 116 lost a camera during an EVA During an STS 120 EVA to reinforce a torn solar panel a pair of pliers was lost and in an STS 126 EVA Heidemarie Stefanyshyn Piper lost a briefcase sized tool bag 78 Boosters Edit Main category Spacecraft that broke apart in space Spent upper stage of a Delta II rocket photographed by the XSS 10 satellite Rocket upper stages which end up in orbit are a significant source of space debris In characterizing the problem of space debris it was learned that much debris was due to rocket upper stages e g the Inertial Upper Stage which end up in orbit and break up due to decomposition of unvented unburned fuel 79 The first such instance involved the launch of the Transit 4a satellite in 1961 Two hours after insertion the Ablestar upper stage exploded But even boosters that don t break apart can be a problem as a major known impact event involved an intact Ariane booster 55 2 Although NASA and the United States Air Force now require upper stage passivation other launchers such as the Chinese and Russian space agencies do not Lower stages like the Space Shuttle s solid rocket boosters or Apollo program s Saturn IB launch vehicles do not reach orbit 80 Orbit of 2020 SO Examples Two Japanese H 2A rockets rockets broke up in 2006 81 A Russian Briz M booster stage exploded in orbit over South Australia on 19 February 2007 Launched on 28 February 2006 carrying an Arabsat 4A communications satellite it malfunctioned before it could use up its propellant Although the explosion was captured on film by astronomers due to the orbit path the debris cloud has been difficult to measure with radar By 21 February 2007 over 1 000 fragments were identified 82 83 A 14 February 2007 breakup was recorded by Celestrak 84 Another Briz M broke up on 16 October 2012 after a failed 6 August Proton M launch The amount and size of the debris was unknown 85 The second stage of the Zenit 2 called the SL 16 by western governments along with the second stages of the Vostok and Kosmos launch vehicles make up about 20 of the total mass of launch debris in Low Earth Orbit LEO 86 An analysis that determined the 50 statistically most concerning debris objects in low Earth orbit determined that the top 20 were all Zenit 2 upper stages 87 a Delta II rocket used to launch NASA s 1989 COBE spacecraft exploded on December 3 2006 This occurred even though its residual fuel had already been vented to space 81 In 2018 2019 three different Atlas V Centaur second stages broke up 88 89 90 In December 2020 scientists confirmed that a previously detected near Earth object 2020 SO was rocket booster space junk launched in 1966 orbiting Earth and the Sun 91 At least eight Delta rockets have contributed orbital debris in the sun synchronous low earth orbit environment The variant of the Delta upper stage that was used in the 1970 s was found to be prone to in orbit explosions Starting in 1981 depletion burns to get rid of excess propellant became standard and no Delta Rocket Bodies launched after 1981 experience severe fragmentations afterward but some of those launched prior to 1981 continued to explode In 1991 the Delta 1975 052B fragmented 16 years after launch demonstrating the resilience of the propellent 92 Weapons Edit Main category Intentionally destroyed artificial satellites A past debris source was the testing of anti satellite weapons ASATs by the U S and Soviet Union during the 1960s and 1970s North American Aerospace Defense Command NORAD files only contained data for Soviet tests and debris from U S tests were only identified later 93 By the time the debris problem was understood widespread ASAT testing had ended the U S Program 437 was shut down in 1975 94 The U S restarted their ASAT programs in the 1980s with the Vought ASM 135 ASAT A 1985 test destroyed a 1 tonne 2 200 lb satellite orbiting at 525 km 326 mi creating thousands of debris larger than 1 cm 0 39 in Due to the altitude atmospheric drag decayed the orbit of most debris within a decade A de facto moratorium followed the test 95 Known orbit planes of Fengyun 1C debris one month after the weather satellite s disintegration by the Chinese ASAT China s government was condemned for the military implications and the amount of debris from the 2007 anti satellite missile test 96 the largest single space debris incident in history creating over 2 300 pieces golf ball size or larger over 35 000 1 cm 0 4 in or larger and one million pieces 1 mm 0 04 in or larger The target satellite orbited between 850 km 530 mi and 882 km 548 mi the portion of near Earth space most densely populated with satellites 97 Since atmospheric drag is low at that altitude the debris is slow to return to Earth and in June 2007 NASA s Terra environmental spacecraft maneuvered to avoid impact from the debris 98 Dr Brian Weeden U S Air Force officer and Secure World Foundation staff member noted that the 2007 Chinese satellite explosion created an orbital debris of more than 3 000 separate objects that then required tracking 99 On 20 February 2008 the U S launched an SM 3 missile from the USS Lake Erie to destroy a defective U S spy satellite thought to be carrying 450 kg 1 000 lb of toxic hydrazine propellant The event occurred at about 250 km 155 mi and the resulting debris has a perigee of 250 km 155 mi or lower 100 The missile was aimed to minimize the amount of debris which according to Pentagon Strategic Command chief Kevin Chilton had decayed by early 2009 101 On 27 March 2019 Indian Prime Minister Narendra Modi announced that India shot down one of its own LEO satellites with a ground based missile He stated that the operation part of Mission Shakti would defend the country s interests in space Afterwards US Air Force Space Command announced they were tracking 270 new pieces of debris but expected the number to grow as data collection continues 102 On 15 November 2021 the Russian Defense Ministry destroyed Kosmos 1408 103 orbiting at around 450 km creating more than 1 500 pieces of trackable debris and hundreds of thousands of pieces of un trackable debris according to the US State Department 104 The vulnerability of satellites to debris and the possibility of attacking LEO satellites to create debris clouds has triggered speculation that it is possible for countries unable to make a precision attack clarification needed An attack on a satellite of 10 t 22 000 lb or more would heavily damage the LEO environment 95 Hazards Edit A micrometeoroid left this crater on the surface of Space Shuttle Challenger s front window on STS 7 To spacecraft Edit Space junk can be a hazard to active satellites and spacecraft It has been theorized that Earth orbit could even become impassable if the risk of collision grows too high 105 failed verification However since the risk to spacecraft increases with exposure to high debris densities it is more accurate to say that LEO would be rendered unusable by orbiting craft The threat to craft passing through LEO to reach a higher orbit would be much lower owing to the very short time span of the crossing Uncrewed spacecraft Edit Although spacecraft are typically protected by Whipple shields solar panels which are exposed to the Sun wear from low mass impacts Even small impacts can produce a cloud of plasma which is an electrical risk to the panels 106 Satellites are believed to have been destroyed by micrometeorites and small orbital debris MMOD The earliest suspected loss was of Kosmos 1275 which disappeared on 24 July 1981 a month after launch Kosmos contained no volatile fuel therefore there appeared to be nothing internal to the satellite which could have caused the destructive explosion which took place However the case has not been proven and another hypothesis forwarded is that the battery exploded Tracking showed it broke up into 300 new objects 107 Many impacts have been confirmed since For example on 24 July 1996 the French microsatellite Cerise was hit by fragments of an Ariane 1 H 10 upper stage booster which exploded in November 1986 55 2 On 29 March 2006 the Russian Ekspress AM11 communications satellite was struck by an unknown object and rendered inoperable 64 On 13 October 2009 Terra suffered a single battery cell failure anomaly and a battery heater control anomaly which were subsequently considered likely the result of an MMOD strike 108 On 12 March 2010 Aura lost power from one half of one of its 11 solar panels and this was also attributed to an MMOD strike 109 On 22 May 2013 GOES 13 was hit by an MMOD which caused it to lose track of the stars that it used to maintain an operational attitude It took nearly a month for the spacecraft to return to operation 110 The first major satellite collision occurred on 10 February 2009 The 950 kg 2 090 lb derelict satellite Kosmos 2251 and the operational 560 kg 1 230 lb Iridium 33 collided 500 mi 800 km 111 over northern Siberia The relative speed of impact was about 11 7 km s 7 3 mi s or about 42 120 km h 26 170 mph 112 Both satellites were destroyed creating thousands of pieces of new smaller debris with legal and political liability issues unresolved even years later 113 114 115 On 22 January 2013 BLITS a Russian laser ranging satellite was struck by debris suspected to be from the 2007 Chinese anti satellite missile test changing both its orbit and rotation rate 116 Satellites sometimes clarification needed perform Collision Avoidance Maneuvers and satellite operators may monitor space debris as part of maneuver planning For example in January 2017 the European Space Agency made the decision to alter orbit of one of its three 117 Swarm mission spacecraft based on data from the US Joint Space Operations Center to lower the risk of collision from Cosmos 375 a derelict Russian satellite 118 Crewed spacecraft Edit Crewed flights are naturally particularly sensitive to the hazards that could be presented by space debris conjunctions in the orbital path of the spacecraft Examples of occasional avoidance maneuvers or longer term space debris wear have occurred in Space Shuttle missions the MIR space station and the International Space Station Space Shuttle missions Edit Space Shuttle Discovery s lower starboard wing and Thermal Protection System tiles photographed on STS 114 during an R Bar Pitch Manoeuvre where astronauts examine the TPS for any damage during ascent From the early Space Shuttle missions NASA used NORAD space monitoring capabilities to assess the Shuttle s orbital path for debris In the 1980s this used a large proportion of NORAD capacity 28 The first collision avoidance maneuver occurred during STS 48 in September 1991 119 a seven second thruster burn to avoid debris from the derelict satellite Kosmos 955 120 Similar maneuvers were initiated on missions 53 72 and 82 119 One of the earliest events to publicize the debris problem occurred on Space Shuttle Challenger s second flight STS 7 A fleck of paint struck its front window creating a pit over 1 mm 0 04 in wide On STS 59 in 1994 Endeavour s front window was pitted about half its depth Minor debris impacts increased from 1998 121 Window chipping and minor damage to thermal protection system tiles TPS were already common by the 1990s The Shuttle was later flown tail first to take a greater proportion of the debris load on the engines and rear cargo bay which are not used in orbit or during descent and thus are less critical for post launch operation When flying attached to the ISS the two connected spacecraft were flipped around so the better armoured station shielded the orbiter 122 Space Shuttle Endeavour had a major impact on its radiator during STS 118 The entry hole is about 5 5 mm 0 22 in and the exit hole is twice as large A NASA 2005 study concluded that debris accounted for approximately half of the overall risk to the Shuttle 122 123 Executive level decision to proceed was required if the catastrophic impact was likelier than 1 in 200 On a normal low orbit mission to the ISS the risk was approximately 1 in 300 but the Hubble telescope repair mission was flown at the higher orbital altitude of 560 km 350 mi where the risk was initially calculated at a 1 in 185 due in part to the 2009 satellite collision A re analysis with better debris numbers reduced the estimated risk to 1 in 221 and the mission went ahead 124 Debris incidents continued on later Shuttle missions During STS 115 in 2006 a fragment of circuit board bored a small hole through the radiator panels in Atlantis s cargo bay 125 On STS 118 in 2007 debris blew a bullet like hole through Endeavour s radiator panel 126 Mir Edit Impact wear was notable on Mir the Soviet space station since it remained in space for long periods with its original solar module panels 127 128 Debris impacts on Mir s solar panels degraded their performance The damage is most noticeable on the panel on the right which is facing the camera with a high degree of contrast Extensive damage to the smaller panel below is due to impact with a Progress spacecraft International Space Station Edit The ISS also uses Whipple shielding to protect its interior from minor debris 129 However exterior portions notably its solar panels cannot be protected easily In 1989 the ISS panels were predicted to degrade approximately 0 23 in four years due to the sandblasting effect of impacts with small orbital debris 130 An avoidance maneuver is typically performed for the ISS if there is a greater than one in 10 000 chance of a debris strike 131 As of January 2014 update there have been sixteen maneuvers in the fifteen years the ISS had been in orbit 131 By 2019 over 1 400 meteoroid and orbital debris MMOD impacts had been recorded on the ISS 132 As another method to reduce the risk to humans on board ISS operational management asked the crew to shelter in the Soyuz on three occasions due to late debris proximity warnings In addition to the sixteen thruster firings and three Soyuz capsule shelter orders one attempted maneuver was not completed due to not having the several days warning necessary to upload the maneuver timeline to the station s computer 131 133 134 A March 2009 event involved debris believed to be a 10 cm 3 9 in piece of the Kosmos 1275 satellite 135 In 2013 the ISS operations management did not make a maneuver to avoid any debris after making a record four debris maneuvers the previous year 131 Kessler syndrome Edit Main article Kessler syndrome Growth of tracked objects in orbit and related events 136 efforts to manage outer space global commons have so far not reduced the debris or the growth of objects in orbit The Kessler syndrome 137 138 proposed by NASA scientist Donald J Kessler in 1978 is a theoretical scenario in which the density of objects in low Earth orbit LEO is high enough that collisions between objects could cause a cascade effect where each collision generates space debris that increases the likelihood of further collisions 139 He further theorized that one implication if this were to occur is that the distribution of debris in orbit could render space activities and the use of satellites in specific orbital ranges economically impractical for many generations 139 The growth in the number of objects as a result of the late 1990s studies sparked debate in the space community on the nature of the problem and the earlier dire warnings According to Kessler s 1991 derivation and 2001 updates 140 the LEO environment in the 1 000 km 620 mi altitude range should be cascading However only one major satellite collision incident occurred the 2009 satellite collision between Iridium 33 and Cosmos 2251 The lack of obvious short term cascading has led to speculation that the original estimates overstated the problem 141 According to Kessler in 2010 however a cascade may not be obvious until it is well advanced which might take years 142 On Earth Edit Main article List of space debris fall incidents Saudi officials inspect a crashed PAM D module in January 2001 Although most debris burns up in the atmosphere larger debris objects can reach the ground intact According to NASA an average of one cataloged piece of debris has fallen back to Earth each day for the past 50 years Despite their size there has been no significant property damage from the debris 143 Burning up in the atmosphere may also contribute to atmospheric pollution 144 Numerous small cylindrical tanks from space objects have been found designed to hold fuel or gasses 145 Tracking and measurement EditSee also Satellite tracking Tracking from the ground Edit Radar and optical detectors such as lidar are the main tools for tracking space debris Although objects under 10 cm 4 in have reduced orbital stability debris as small as 1 cm can be tracked 146 147 however determining orbits to allow re acquisition is difficult Most debris remain unobserved The NASA Orbital Debris Observatory tracked space debris with a 3 m 10 ft liquid mirror transit telescope 148 FM Radio waves can detect debris after reflecting off them onto a receiver 149 Optical tracking may be a useful early warning system on spacecraft 150 The U S Strategic Command keeps a catalog of known orbital objects using ground based radar and telescopes and a space based telescope originally to distinguish from hostile missiles The 2009 edition listed about 19 000 objects 151 Other data come from the ESA Space Debris Telescope TIRA 152 the Goldstone Haystack 153 and EISCAT radars and the Cobra Dane phased array radar 154 to be used in debris environment models like the ESA Meteoroid and Space Debris Terrestrial Environment Reference MASTER Measurement in space Edit The Long Duration Exposure Facility LDEF is an important source of information on small particle space debris Returned space hardware is a valuable source of information on the directional distribution and composition of the sub millimetre debris flux The LDEF satellite deployed by mission STS 41 C Challenger and retrieved by STS 32 Columbia spent 68 months in orbit to gather debris data The EURECA satellite deployed by STS 46 Atlantis in 1992 and retrieved by STS 57 Endeavour in 1993 was also used for debris study 155 The solar arrays of Hubble were returned by missions STS 61 Endeavour and STS 109 Columbia and the impact craters studied by the ESA to validate its models Materials returned from Mir were also studied notably the Mir Environmental Effects Payload which also tested materials intended for the ISS 156 157 158 Gabbard diagrams Edit A debris cloud resulting from a single event is studied with scatter plots known as Gabbard diagrams where the perigee and apogee of fragments are plotted with respect to their orbital period Gabbard diagrams of the early debris cloud prior to the effects of perturbations if the data were available are reconstructed They often include data on newly observed as yet uncatalogued fragments Gabbard diagrams can provide important insights into the features of the fragmentation the direction and point of impact 23 159 Dealing with debris EditAn average of about one tracked object per day has been dropping out of orbit for the past 50 years 160 averaging almost three objects per day at solar maximum due to the heating and expansion of the Earth s atmosphere but one about every three days at solar minimum usually five and a half years later 160 In addition to natural atmospheric effects corporations academics and government agencies have proposed plans and technology to deal with space debris but as of November 2014 update most of these are theoretical and there is no extant business plan for debris reduction 24 A number of scholars have also observed that institutional factors political legal economic and cultural rules of the game are the greatest impediment to the cleanup of near Earth space There is little commercial incentive to act since costs are not assigned to polluters though a number of technological solutions have been suggested 24 However effects to date are limited In the US governmental bodies have been accused of backsliding on previous commitments to limit debris growth let alone tackling the more complex issues of removing orbital debris 161 The different methods for removal of space debris have been evaluated by the Space Generation Advisory Council including French astrophysicist Fatoumata Kebe 162 Growth mitigation Edit See also Space traffic management Spatial density of LEO space debris by altitude according to 2011 a NASA report to the United Nations Office for Outer Space Affairs 163 Spatial density of space debris by altitude according to ESA MASTER 2001 without debris from the Chinese ASAT and 2009 collision events As of the 2010s several technical approaches to the mitigation of the growth of space debris are typically undertaken yet no comprehensive legal regime or cost assignment structure is in place to reduce space debris in the way that terrestrial pollution has reduced since the mid 20th century To avoid excessive creation of artificial space debris many but not all satellites launched to above low Earth orbit are launched initially into elliptical orbits with perigees inside Earth s atmosphere so the orbit will quickly decay and the satellites then will destroy themselves upon reentry into the atmosphere Other methods are used for spacecraft in higher orbits These include passivation of the spacecraft at the end of its useful life as well as the use of upper stages that can reignite to decelerate the stage to intentionally deorbit it often on the first or second orbit following payload release satellites that can if they remain healthy for years deorbit themselves from the lower orbits around Earth Other satellites such as many CubeSats in low orbits below approximately 400 km 250 mi orbital altitude depend on the energy absorbing effects of the upper atmosphere to reliably deorbit a spacecraft within weeks or months Increasingly spent upper stages in higher orbits orbits for which low delta v deorbit is not possible or not planned for and architectures that support satellite passivation at end of life are passivated at end of life This removes any internal energy contained in the vehicle at the end of its mission or useful life While this does not remove the debris of the now derelict rocket stage or satellite itself it does substantially reduce the likelihood of the spacecraft destructing and creating many smaller pieces of space debris a phenomenon that was common in many of the early generations of US and Soviet 71 spacecraft Upper stage passivation e g of Delta boosters 28 by releasing residual propellants reduces debris from orbital explosions however even as late as 2011 not all upper stages implement this practice 164 SpaceX used the term propulsive passivation for the final maneuver of their six hour demonstration mission STP 2 of the Falcon 9 second stage for the US Air Force in 2019 but did not define what all that term encompassed 165 With a one up one down launch license policy for Earth orbits launchers would rendezvous with capture and de orbit a derelict satellite from approximately the same orbital plane 166 Another possibility is the robotic refueling of satellites Experiments have been flown by NASA 167 and SpaceX is developing large scale on orbit propellant transfer technology 168 Another approach to debris mitigation is to explicitly design the mission architecture to always leave the rocket second stage in an elliptical geocentric orbit with a low perigee thus ensuring rapid orbital decay and avoiding long term orbital debris from spent rocket bodies Such missions will often complete the payload placement in a final orbit by the use of low thrust electric propulsion or with the use of a small kick stage to circularize the orbit The kick stage itself may be designed with the excess propellant capability to be able to self deorbit 169 Self removal Edit Although the ITU requires geostationary satellites to move to a graveyard orbit at the end of their lives the selected orbital areas do not sufficiently protect GEO lanes from debris 60 Rocket stages or satellites with enough propellant may make a direct controlled de orbit or if this would require too much propellant a satellite may be brought to an orbit where atmospheric drag would cause it to eventually de orbit This was done with the French Spot 1 satellite reducing its atmospheric re entry time from a projected 200 years to about 15 by lowering its altitude from 830 km 516 mi to about 550 km 342 mi 170 171 The Iridium constellation 95 communication satellites launched during the five year period between 1997 and 2002 provides a set of data points on the limits of self removal The satellite operator Iridium Communications remained operational over the two decade life of the satellites albeit with a company name change through a corporate bankruptcy during the period and by December 2019 had completed disposal of the last of its 65 working legacy satellites 172 However this process left 30 satellites with a combined mass of 20 400 kg 45 000 lb or nearly a third of the mass of this constellation in LEO orbits at approximately 700 km 430 mi altitude where self decay is quite slow Of these satellites 29 simply failed during their time in orbit and were thus unable to self deorbit while one Iridium 33 was involved in the 2009 satellite collision with the derelict Russian military satellite Kosmos 2251 172 No contingency plan was laid for the removal of satellites that were unable to remove themselves In 2019 the Iridium CEO Matt Desch said that Iridium would be willing to pay an active debris removal company to deorbit its remaining first generation satellites if it were possible for an unrealistically low cost say US 10 000 per deorbit but he acknowledged that price would likely be far below what a debris removal company could realistically offer You know at what point it s a no brainer but I expect the cost is really in the millions or tens of millions at which price I know it doesn t make sense 172 Passive methods of increasing the orbital decay rate of spacecraft debris have been proposed Instead of rockets an electrodynamic tether could be attached to a spacecraft at launch at the end of its lifetime the tether would be rolled out to slow the spacecraft 173 Other proposals include a booster stage with a sail like attachment 174 and a large thin inflatable balloon envelope 175 In late December 2022 ESA successfully carried out a demonstration of a breaking sail based satellite deorbiter ADEO which could be used by mitigation measures and is part of ESA s Zero Debris Initiative Around one year earlier China also tested a drag sail 176 177 External removal Edit A variety of approaches have been proposed studied or had ground subsystems built to use other spacecraft to remove existing space debris A consensus of speakers at a meeting in Brussels in October 2012 organized by the Secure World Foundation a U S think tank and the French International Relations Institute 178 reported that removal of the largest debris would be required to prevent the risk to spacecraft becoming unacceptable in the foreseeable future without any addition to the inventory of dead spacecraft in LEO To date in 2019 removal costs and legal questions about ownership and the authority to remove defunct satellites have stymied national or international action Current space law retains ownership of all satellites with their original operators even debris or spacecraft which are defunct or threaten active missions Multiple companies made plans in the late 2010s to conduct external removal on their satellites in mid LEO orbits For example OneWeb planned to utilize onboard self removal as plan A for satellite deorbiting at the end of life but if a satellite were unable to remove itself within one year of end of life OneWeb would implement plan B and dispatch a reusable multi transport mission space tug to attach to the satellite at an already built in capture target via a grappling fixture to be towed to a lower orbit and released for re entry 179 180 Remotely controlled vehicles Edit A well studied solution uses a remotely controlled vehicle to rendezvous with capture and return debris to a central station 181 One such system is Space Infrastructure Servicing a commercially developed refueling depot and service spacecraft for communications satellites in geosynchronous orbit originally scheduled for a 2015 launch 182 The SIS would be able to push dead satellites into graveyard orbits 183 The Advanced Common Evolved Stage family of upper stages is being designed with a high leftover propellant margin for derelict capture and de orbit and in space refueling capability for the high delta v required to de orbit heavy objects from geosynchronous orbit 166 A tug like satellite to drag debris to a safe altitude for it to burn up in the atmosphere has been researched 184 When debris is identified the satellite creates a difference in potential between the debris and itself then using its thrusters to move itself and the debris to a safer orbit A variation of this approach is for the remotely controlled vehicle to rendezvous with debris capture it temporarily to attach a smaller de orbit satellite and drag the debris with a tether to the desired location The mothership would then tow the debris smallsat combination for atmospheric entry or move it to a graveyard orbit One such system is the proposed Busek ORbital DEbris Remover ORDER which would carry over 40 SUL satellite on umbilical line de orbit satellites and propellant sufficient for their removal 24 On 7 January 2010 Star Inc reported that it received a contract from the Space and Naval Warfare Systems Command for a feasibility study of the ElectroDynamic Debris Eliminator EDDE propellantless spacecraft for space debris removal 185 In February 2012 the Swiss Space Center at Ecole Polytechnique Federale de Lausanne announced the Clean Space One project a nanosatellite demonstration project for matching orbit with a defunct Swiss nanosatellite capturing it and de orbiting together 186 The mission has seen several evolutions to reach a pac man inspired capture model 187 In 2013 Space Sweeper with Sling Sat 4S a grappling satellite which captures and ejects debris was studied 188 needs update In 2022 a Chinese satellite SJ 21 grabbed an unused satellite and threw it into an orbit with a lower risk for it to collide 189 190 In December 2019 the European Space Agency awarded the first contract to clean up space debris The 120 million mission dubbed ClearSpace 1 a spinoff from the EPFL project is slated to launch in 2025 It aims to remove a 100 kg VEga Secondary Payload Adapter Vespa 191 left by Vega flight VV02 in an 800 km 500 mi orbit in 2013 A chaser will grab the junk with four robotic arms and drag it down to Earth s atmosphere where both will burn up 192 Laser methods Edit The laser broom uses a ground based laser to ablate the front of the debris producing a rocket like thrust that slows the object With continued application the debris would fall enough to be influenced by atmospheric drag 193 194 During the late 1990s the U S Air Force s Project Orion was a laser broom design 195 Although a test bed device was scheduled to launch on a Space Shuttle in 2003 international agreements banning powerful laser testing in orbit limited its use to measurements 196 The 2003 Space Shuttle Columbia disaster postponed the project and according to Nicholas Johnson chief scientist and program manager for NASA s Orbital Debris Program Office There are lots of little gotchas in the Orion final report There s a reason why it s been sitting on the shelf for more than a decade 197 The momentum of the laser beam photons could directly impart a thrust on the debris sufficient to move small debris into new orbits out of the way of working satellites NASA research in 2011 indicates that firing a laser beam at a piece of space junk could impart an impulse of 1 mm 0 039 in per second and keeping the laser on the debris for a few hours per day could alter its course by 200 m 660 ft per day 198 One drawback is the potential for material degradation the energy may break up the debris adding to the problem 199 A similar proposal places the laser on a satellite in Sun synchronous orbit using a pulsed beam to push satellites into lower orbits to accelerate their reentry 24 A proposal to replace the laser with an Ion Beam Shepherd has been made 200 and other proposals use a foamy ball of aerogel or a spray of water 201 inflatable balloons 202 electrodynamic tethers 203 electroadhesion 204 and dedicated anti satellite weapons 205 Nets Edit On 28 February 2014 Japan s Japan Aerospace Exploration Agency JAXA launched a test space net satellite The launch was an operational test only 206 In December 2016 the country sent a space junk collector via Kounotori 6 to the ISS by which JAXA scientists experiment to pull junk out of orbit using a tether 207 208 The system failed to extend a 700 meter tether from a space station resupply vehicle that was returning to Earth 209 210 On 6 February the mission was declared a failure and leading researcher Koichi Inoue told reporters that they believe the tether did not get released 211 Since 2012 the European Space Agency has been working on the design of a mission to remove large space debris from orbit The mission e Deorbit is scheduled for launch during 2023 with an objective to remove debris heavier than 4 000 kilograms 8 800 lb from LEO 212 Several capture techniques are being studied including a net a harpoon and a combination robot arm and clamping mechanism 213 Harpoon Edit The RemoveDEBRIS mission plan is to test the efficacy of several ADR technologies on mock targets in low Earth orbit In order to complete its planned experiments the platform is equipped with a net a harpoon a laser ranging instrument a dragsail and two CubeSats miniature research satellites 214 The mission was launched on 2 April 2018 National and international regulation Edit There is no international treaty minimizing space debris However the United Nations Committee on the Peaceful Uses of Outer Space COPUOS published voluntary guidelines in 2007 215 using a variety of earlier national regulatory attempts at developing standards for debris mitigation As of 2008 the committee was discussing international rules of the road to prevent collisions between satellites 216 By 2013 a number of national legal regimes existed 217 218 219 typically instantiated in the launch licenses that are required for a launch in all spacefaring nations 220 The U S issued a set of standard practices for civilian NASA and military DoD and USAF orbital debris mitigation in 2001 221 222 218 The standard envisioned disposal for final mission orbits in one of three ways 1 atmospheric reentry where even with conservative projections for solar activity atmospheric drag will limit the lifetime to no longer than 25 years after completion of mission 2 maneuver to a storage orbit move the spacecraft to one of four very broad parking orbit ranges 2 000 19 700 km 1 200 12 200 mi 20 700 35 300 km 12 900 21 900 mi above 36 100 km 22 400 mi or out of Earth orbit completely and into any heliocentric orbit 3 Direct retrieval Retrieve the structure and remove it from orbit as soon as practicable after completion of mission 217 The standard articulated in option 1 which is the standard applicable to most satellites and derelict upper stages launched has come to be known as the 25 year rule 223 The US updated the Orbital Debris Mitigation Standard Practices ODMSP in December 2019 but made no change to the 25 year rule even though m any in the space community believe that the timeframe should be less than 25 years 224 There is no consensus however on what any new timeframe might be 224 In 2002 the European Space Agency ESA worked with an international group to promulgate a similar set of standards also with a 25 year rule applying to most Earth orbit satellites and upper stages Space agencies in Europe began to develop technical guidelines in the mid 1990s and ASI UKSA CNES DLR and ESA signed a European Code of Conduct in 2006 219 which was a predecessor standard to the ISO international standard work that would begin the following year In 2008 ESA further developed its own Requirements on Space Debris Mitigation for Agency Projects which came into force on 1 April 2008 219 Germany and France have posted bonds to safeguard the property from debris damage clarification needed 225 The direct retrieval option option no 3 in the US standard practices above has rarely been done by any spacefaring nation exception USAF X 37 or commercial actor since the earliest days of spaceflight due to the cost and complexity of achieving direct retrieval but the ESA has scheduled a 2025 demonstration mission Clearspace 1 to do this with a single small 100 kg 220 lb derelict upper stage at a projected cost of 120 million not including the launch costs 192 By 2006 the Indian Space Research Organization ISRO had developed a number of technical means of debris mitigation upper stage passivation propellant reserves for movement to graveyard orbits etc for ISRO launch vehicles and satellites and was actively contributing to inter agency debris coordination and the efforts of the UN COPUOS committee 226 In 2007 the ISO began preparing an international standard for space debris mitigation 227 By 2010 ISO had published a comprehensive set of space system engineering standards aimed at mitigating space debris with primary requirements defined in the top level standard ISO 24113 By 2017 the standards were nearly complete However these standards are not binding on any party by ISO or any international jurisdiction They are simply available for use in any of a variety of voluntary ways They can be adopted voluntarily by a spacecraft manufacturer or operator or brought into effect through a commercial contract between a customer and supplier or used as the basis for establishing a set of national regulations on space debris mitigation 223 The voluntary ISO standard also adopted the 25 year rule for the LEO protected region below 2 000 km 1 200 mi altitude that has been previously and still is as of 2019 update used by the US ESA and UN mitigation standards and identifies it as an upper limit for the amount of time that a space system shall remain in orbit after its mission is completed Ideally the time to deorbit should be as short as possible i e much shorter than 25 years 223 Holger Krag of the European Space Agency states that as of 2017 there is no binding international regulatory framework with no progress occurring at the respective UN body in Vienna 105 Barriers Edit With the rapid development of the computer and digitalization industries more countries and companies have engaged in space activities since the turn of the 20th century The tragedy of the commons is an economic theory referring to a situation where maximizing self interest through using a shared resource can finally lead to the resource degradation shared by all 228 Based on the theory individuals rational action in space will finally lead to an irrational collective result orbits are crowded with debris As a common pool resource the Earth s orbits especially LEO and GEO that accommodate most satellites are nonexcludable and rivalry 229 To address the tragedy and ensure space sustainability many technical approaches have been developed And in terms of governance mechanisms the top down centralized one is less suitable to tackle the complex debris problem due to the increasing number of space actors 230 Instead much evidence has proved that polycentric form of governance developed by Elinor Ostrom can work in space 231 In the process of promoting the polycentric network there are some existing barriers needed to be dealt with Incomplete data of space debris Edit As orbital debris is a global problem affecting both spacefaring and non spacefaring nations it is necessary to be handled in a worldwide context 228 Because of the complexity and dynamics of object movements like spacecrafts debris meteorites etc many countries and regions including the United States Europe Russia and China have developed their space situational awareness SSA to avoid potential threats in space or plan actions in advance 232 To a certain extent SSA plays a role in tracking space debris In order to build a powerful SSA system there are two prerequisites international cooperation and exchange of information and data 232 However limitations still exist in spite of the substantially improving data quality over the past decades Some space powers are not willing to share the information that they have collected and those such as the U S that have shared the data keep parts of it secret 233 Instead of joining in a coordinated way a great deal of SSA programs and national databases run parallel to each other with some overlaps hindering the formation of a collaborative monitoring system 233 Some private actors are also trying to establish SSA systems For example the Space Data Association SDA formed in 2009 is a non governmental entity It currently consists of 21 global satellite operators and 4 executive members Eutelsat Inmarsat Intelsat and SES SDA is a non profit platform aiming to avoid radio interference and space collisions through pooling data from operators independently 232 Researchers suggest that it is essential to establish an international center for exchanging information on space debris because SSA networks do not completely equal debris tracking systems the former ones focus more on active and threatening objects in space 234 And in terms of debris populations and defunct satellites not very much operators have provided data 234 In a polycentric governance network a resource that cannot be holistically monitored is less possible to be well managed 233 Both insufficient transnational cooperation and information sharing bring resistance to addressing the debris problem There is still a long way to go before building a global network that covers complete data and has strong interconnection and interoperability Insufficient participation of private actors Edit With the commercialization of satellites and space the private sector is getting more interested in space activities For example SpaceX is planning to create a network of around 12 000 small satellites that can transmit high speed internet to any place in the world 235 The proportion of commercial spacecrafts has increased from 4 6 in the 1980s to 55 6 in the 2010s 236 Despite the high participation rate of commercial entities UN COPUOS once deliberately excluded them from having a voice in discussions unless being formally invited by a member state 230 Ostrom said that the involvement of all relevant stakeholders in the rule design and implementation process is one of the critical elements of successful governance 237 The exclusion of private actors largely reduces the effectiveness of the committee s role in making collective choice arrangements that reflect the interests of all space users 230 The limited engagement of private actors slows down the process of addressing space debris to some degree 238 Ties existing between dissimilar stakeholders in the governance network offer access to diverse resources 239 Different competence among stakeholders can help allocate the tasks more reasonably In that case the expertise and experience of private operators are critical to help the world achieve space sustainability 238 The complementary strengths of different stakeholders enable the governance network to be more adaptable to changes and reach common goals more effectively 239 In recent years many private actors have seen commercial opportunities of eliminating space debris It is estimated that by 2022 the global market for debris monitoring and removal will generate a revenue of around 2 9 billion 240 For example Astroscale has contracted with European and Japanese space agencies to develop the capacity of removing orbital debris 241 Despite that they are still in small quantity compared to the number of those who have placed satellites in space Privateer Space a Hawaiian based startup company started by American engineer Alex Fielding space environmentalist Dr Moriba Jah and Apple co founder Steve Wozniak announced plans in September 2021 to launch hundreds of satellites into orbit in order to study space debris 242 However the company stated it is in stealth mode and no such satellites have been launched 242 Fortunately the current space exploration is not completely driven by competition and there still exists a chance for dialogues and cooperation among all stakeholders in both developed and developing countries to reach an agreement on tackling space debris and assure an equitable and orderly exploration 243 Besides private actors network governance does not necessarily exclude the states from playing a role Instead the different functions of states might promote the governance process 244 To improve the polycentric governance network of space debris researchers suggest encourage data sharing among different national and organizational databases at the political level develop shared standards for data collection systems to improve interoperability enhance the participation of private actors through involving them in national and international discussions 233 Environmental concerns Edit The continued practice of disposing of space debris on Earth in areas such as the spacecraft cemetery has raised environmental concerns 245 Klinger states that the environmental geopolitics of Earth and outer space are inextricably linked by the spatial politics of privilege and sacrifice among people places and institutions 245 246 Since 1971 273 spacecraft and satellites have been directed to Point Nemo this number includes the Mir Space Station 142 tonnes and will include the International Space Station in 2024 240 tonnes In 2018 it was found that the water had 26 microplastic particles per cubic metre meaning it is highly polluted 247 The prevalence of orbital debris has been likened to the terrestrial environmental phenomenon of sacrifice zones which are designated geographic regions with high levels of environmental degradation Since the 1960s over three hundred rocket launch sites have been built globally 245 Among these launch sites 17 hosted 90 launches in 2017 alone 245 Rocket launches affect local and global environments through the construction of necessary infrastructure exposure of local environments to toxic residue and the dispersal of pollutants 245 Rockets are the only source of direct anthropogenic emissions into the stratosphere and emit ozone depleting substances such as nitrous oxide hydrogen chloride and aluminium oxide these substances can destroy 105 ozone molecules before depleting 245 Each launch showers an area concentrated within a kilometre with toxins heavy metals and acids 245 This results in localised regional acid rain plant death fish kills and failed seed germination 245 Furthermore studies on trace elements concentration in alligators near NASA launch activities in Florida USA showed that over 50 of alligators had greater than toxic levels of trace elements in their liver 245 Similarly research in Kazakhstan Russia and China has found that unsymmetrical dimethylhydrazine UDMH has carcinogenic mutagenic convulsant teratogenic embryotoxic and DNA damaging effects on rodents living near the Baikonur Cosmodrome Kazakhstan 248 It is unknown however at what trace concentrations these toxic effects manifest in humans or how it may bioaccumulate up the food chain 248 A lack of adequate resourcing to maintain safe non toxic environments makes these areas sacrifice zones and spaces of waste The relative remoteness of these spaces makes them attractive launch sites yet this periphery remain central to both their human and non human inhabitants who become sacrificial 249 250 245 Orbital debris as a question of environmental justice Edit An increase in anthropogenic activity in outer space has resulted in large amounts of physical pollution known as orbital debris 251 This has resulted in space becoming more and more congested due to this rapid increase 252 This increase in congestion threatens the orbital operations of nations and corporations alike 251 However orbital debris also has an impact on the wider population through various means such as potentially lethal debris falling from the sky 253 or orbital debris ruining night skies through light pollution 254 Environmental justice as described by the United States Environmental Protection Agency is the fair and meaningful involvement of all demographics in the development and implementation of environmental regulations and policies 255 Outer space can be seen as an environment like any other environment on Earth 256 making orbital debris a potential issue of environmental justice The idea of environmental injustice is also that the rights of those who have suffered environmental harm or have been disrupted and encroached upon by more powerful actors are protected 256 In the context of the space industry large space organisations and nations are the powerful actors and those who have suffered are public Recent research shows that space exploration opens many questions about environmental justice 257 Environmental geopolitics of the earth and that of outer space are linked particularly by the geopolitics of privilege from one party and sacrifice from another 256 They are also linked in the premise of environmental justice this injustice can unfold on multiple scales such as emission from space launches placement of outer space related infrastructure and of course orbital debris in this case 256 There is an argument that as well as viewing space as an environment space should also be viewed as a commons 258 If space is viewed as a commons then its resources need to be managed for the common good of all people If not then this poses a risk of injustice By managing space as a resource that all nations have access to and none can claim sovereignity over outer space can be also understood as an example of a global commons However legally defining space as a common is challenging as the idea of global commons is a social construct 252 Many space treaties include various phrases describing and defining the usage of outer space including phrases such as for the benefit of all people and shall be the providence of all mankind 259 However none of these treaties provides an adequate framework for handling resources or resolving issues 259 Governance frameworks for outer space have a very narrow and utilitarian view of outer space that looks at what they can gain from exploration 260 At other celestial bodies Edit A piece of a thermal blanket that may have come from the descent stage of the Perseverance Perseverance s backshell sitting upright on the surface of Jezero Crater The issue of space debris has been raised as a mitigation challenge for missions around the Moon with the danger of increasing space debris around it 261 262 In 2022 several elements of space debris were found on Mars Perseverance s backshell was found on the surface of Jezero Crater 263 and a piece of a thermal blanket that may have come from the descent stage of the rover 264 265 It is thought that on 4 March 2022 for the first time human space debris most likely a spent rocket body Long March 3C third stage from the 2014 Chang e 5 T1 mission unintentionally hit the lunar surface creating an unexpected double crater 266 267 In popular culture EditUntil the End of the World 1991 is a French sci fi drama set under the backdrop of an out of control Indian nuclear satellite predicted to re enter the atmosphere threatening vast populated areas of the Earth 268 Gravity a 2013 survival film directed by Alfonso Cuaron is about a disaster on a space mission caused by Kessler syndrome 269 In season 1 of Love Death amp Robots 2019 episode 11 Helping Hand revolves around an astronaut being struck by a screw from space debris which knocks her off a satellite in orbit 270 Manga and anime Planetes tells a story about a crew of Space Debris station that collects and disposes 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14 January 2020 Risks from Orbital Debris and Space Situational Awareness PDF IAA Conference on Space Situational Awareness Washington D C Retrieved 21 January 2023 Schefter Jim July 1982 The Growing Peril of Space Debris Popular Science Vol 221 no 1 pp 48 51 via Google Books Further reading Edit What is Orbital Debris Center for Orbital and Reentry Debris Studies Aerospace Corporation Committee for the Assessment of NASA s Orbital Debris Programs 2011 Limiting Future Collision Risk to Spacecraft An Assessment of NASA s Meteoroid and Orbital Debris Programs Washington D C National Research Council ISBN 978 0 309 21974 7 Klotz Irene 1 September 2011 Space junk reaching tipping point report warns Reuters Retrieved 2 September 2011 News item summarizing the above report Steven A Hildreth and Allison Arnold Threats to U S National Security Interests in Space Orbital Debris Mitigation and Removal Washington D C Congressional Research Service 8 January 2014 David Leonard The Clutter Above Bulletin of the Atomic Scientists July August 2005 Patrick McDaniel A Methodology for Estimating the Uncertainty in the Predicted Annual Risk to Orbiting Spacecraft from Current or Predicted Space Debris Population National Defense University 1997 Interagency Report on Orbital Debris 1995 National Science and Technology Council November 1995 Nickolay Smirnov Space Debris Hazard Evaluation and Mitigation Boca Raton FL CRC Press 2002 ISBN 0 415 27907 0 Richard Talcott How We Junked Up Outer Space Astronomy Volume 36 Issue 6 June 2008 pp 40 43 Technical report on space debris 1999 United Nations 2006 ISBN 92 1 100813 1 Robin Biesbroek 2015 Active Debris Removal in Space How to Clean the Earth s Environment from Space Debris CreateSpace ISBN 978 1 5085 2918 7 Khatchadourian Raffi The Trash Nebula Millions of man made artifacts are circling Earth Will one of them cause a disaster 28 September 2020 pp 44 52 54 55 By one estimate there are a hundred million bits of debris that are a millimetre in size a hundred million as small as a micron We live in a corona of trash T he problem if ignored could destroy all the satellites that orbit near the Earth a loss that would be more acutely felt as humanity increasingly relied on space p 47 External links Edit Wikimedia Commons has media related to Space debris Sativew Tracking Space Junk in real time NASA Orbital Debris Program Office ESA Space Debris Office Archived 5 September 2012 at the Wayback Machine Space the final junkyard documentary film Would a Saturn like ring system around planet Earth remain stable Abdul Ahad EISCAT Space Debris during the international polar year Intro to mathematical modeling of space debris flux Archived 28 February 2019 at the Wayback Machine SOCRATES A free daily service predicting close encounters on orbit between satellites and debris orbiting Earth A summary of current space debris by type and orbit Space Junk Astronomy Cast episode No 82 includes full transcript Paul Maley s Satellite Page Space debris with photos Space Debris Illustrated The Problem in Pictures PACA Space Debris IEEE The Growing Threat of Space Debris The Threat of Orbital Debris and Protecting NASA Space Assets from Satellite Collisions Orbital Debris Space Age Wasteland Debris in Orbit Is Here to Stay Scientific American 2012 United States Space Surveillance Network PATENDER GMV S Trailblazing low gravity space debris capture system Space Junk Infographic Stuff In Space Astria Graph Retrieved from https en wikipedia org w index php title Space debris amp oldid 1154713402, wikipedia, wiki, book, books, library,

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