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2003 SS422

2003 SS422 is a trans-Neptunian object located in the outermost region of the Solar System. It was discovered on 28 September 2003, by American astronomers at the Cerro Tololo Observatory in La Serena, Chile, and estimated to measure approximately 168 kilometers (104 miles) in diameter.[1][3]

2003 SS422
Discovery[1]
Discovered byCerro Tololo Obs.
Discovery siteCerro Tololo Obs.
Discovery date28 September 2003
Designations
2003 SS422
TNO[2] · extreme[3]
distant[1]
Orbital characteristics[4]
Epoch 5 July 2021 (JD 2459400.5)
Uncertainty parameter 3[2]
Observation arc14.92 yr (5,448 days)
Aphelion356.788 AU
Perihelion39.574 AU
198.181 AU
Eccentricity0.8003140
2790 yr
1.770°
0° 0m 1.272s / day
Inclination16.773°
150.949°
206.824°
Physical characteristics
Mean diameter
163 km (est. at 0.09)[3]
7.04[4]

Due to the object's high eccentricity and large perihelia, 2003 SS422 is an extreme trans-Neptunian object from the scattered disc (ESDO).[3] It was a lost minor planet until it was recovered in June 2021.[4]

Orbit and classification edit

Based on an observation arc of 14.9 years with 26 observations in total, 2003 SS422 orbits the Sun at a distance of 39.6–356.8 AU once every 2790 years (1,019,048 days; semi-major axis of 198.2 AU). Its orbit has an eccentricity of 0.80 and an inclination of 17° with respect to the ecliptic.[2]

As of 2021, 2003 SS422 belongs to a small number of 21 high-eccentricity and large-perihelia objects (q > 38 AU) with a semi-major axis of larger than 150 AU,[5] which are the defining orbital parameters of the group of extreme scattered disc object, or ESDO. It is thought that objects cannot reach such orbits without some perturbing object outside the eight planets, which has led to the speculation of Planet Nine.

References edit

  1. ^ a b c "2003 SS422". Minor Planet Center. Retrieved 5 March 2021.
  2. ^ a b c "JPL Small-Body Database Browser: (2003 SS422)" (2020-11-18 last obs.). Jet Propulsion Laboratory. Retrieved 5 March 2021.
  3. ^ a b c d Johnston, Wm. Robert (18 August 2020). "List of Known Trans-Neptunian Objects". Johnston's Archive. Retrieved 5 March 2021.
  4. ^ a b c "MPEC 2021-M14 : 2003 SS422". Minor Planet Center. 16 June 2021. Retrieved 16 June 2021.
  5. ^ "Query (search criteria): objects perihelion min. 38 AU and semimajor axis min. 150 AU (found: 25 objects)". Minor Planet Center. Retrieved 5 March 2021.

External links edit

  • List Of Transneptunian Objects, Minor Planet Center
  • List of Known Trans-Neptunian Objects, Johnston's Archive
  • 2003 SS422 at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

2003, 2003, ss422, trans, neptunian, object, located, outermost, region, solar, system, discovered, september, 2003, american, astronomers, cerro, tololo, observatory, serena, chile, estimated, measure, approximately, kilometers, miles, diameter, 2003, ss422di. 2003 SS422 is a trans Neptunian object located in the outermost region of the Solar System It was discovered on 28 September 2003 by American astronomers at the Cerro Tololo Observatory in La Serena Chile and estimated to measure approximately 168 kilometers 104 miles in diameter 1 3 2003 SS422Discovery 1 Discovered byCerro Tololo Obs Discovery siteCerro Tololo Obs Discovery date28 September 2003DesignationsMPC designation2003 SS422Minor planet categoryTNO 2 extreme 3 distant 1 Orbital characteristics 4 Epoch 5 July 2021 JD 2459400 5 Uncertainty parameter 3 2 Observation arc14 92 yr 5 448 days Aphelion356 788 AUPerihelion39 574 AUSemi major axis198 181 AUEccentricity0 8003140Orbital period sidereal 2790 yrMean anomaly1 770 Mean motion0 0m 1 272s dayInclination16 773 Longitude of ascending node150 949 Argument of perihelion206 824 Physical characteristicsMean diameter163 km est at 0 09 3 Absolute magnitude H 7 04 4 Due to the object s high eccentricity and large perihelia 2003 SS422 is an extreme trans Neptunian object from the scattered disc ESDO 3 It was a lost minor planet until it was recovered in June 2021 4 Orbit and classification editBased on an observation arc of 14 9 years with 26 observations in total 2003 SS422 orbits the Sun at a distance of 39 6 356 8 AU once every 2790 years 1 019 048 days semi major axis of 198 2 AU Its orbit has an eccentricity of 0 80 and an inclination of 17 with respect to the ecliptic 2 As of 2021 update 2003 SS422 belongs to a small number of 21 high eccentricity and large perihelia objects q gt 38 AU with a semi major axis of larger than 150 AU 5 which are the defining orbital parameters of the group of extreme scattered disc object or ESDO It is thought that objects cannot reach such orbits without some perturbing object outside the eight planets which has led to the speculation of Planet Nine References edit a b c 2003 SS422 Minor Planet Center Retrieved 5 March 2021 a b c JPL Small Body Database Browser 2003 SS422 2020 11 18 last obs Jet Propulsion Laboratory Retrieved 5 March 2021 a b c d Johnston Wm Robert 18 August 2020 List of Known Trans Neptunian Objects Johnston s Archive Retrieved 5 March 2021 a b c MPEC 2021 M14 2003 SS422 Minor Planet Center 16 June 2021 Retrieved 16 June 2021 Query search criteria objects perihelion min 38 AU and semimajor axis min 150 AU found 25 objects Minor Planet Center Retrieved 5 March 2021 External links editList Of Transneptunian Objects Minor Planet Center List of Known Trans Neptunian Objects Johnston s Archive 2003 SS422 at the JPL Small Body Database nbsp Close approach Discovery Ephemeris Orbit diagram Orbital elements Physical parameters Retrieved from https en wikipedia org w index php title 2003 SS422 amp oldid 1187131020, wikipedia, wiki, book, books, library,

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