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(12538) 1998 OH

(12538) 1998 OH is a stony asteroid, classified as near-Earth object and potentially hazardous asteroid of the Apollo group, approximately 1.8 kilometers (1.1 miles) in diameter. It was discovered on 19 July 1998, by astronomers of the Near-Earth Asteroid Tracking program at the Haleakala Observatory in Hawaii, United States.[2] In 2019, the asteroid came within about 73 lunar distances of Earth.

(12538) 1998 OH
Discovery[1]
Discovered byNEAT
Discovery siteHaleakala Obs.
Discovery date19 July 1998
Designations
(12538) 1998 OH
1998 OH
NEO · Apollo · PHA[1][2]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc25.96 yr (9,483 days)
Aphelion2.1674 AU
Perihelion0.9155 AU
1.5414 AU
Eccentricity0.4061
1.91 yr (699 days)
58.305°
0° 30m 54s / day
Inclination24.529°
220.75°
321.72°
Earth MOID0.0280 AU · 10.9 LD
Physical characteristics
Dimensions1.663±0.329 km[3][4]
2.06 km (calculated)[5]
2.58±0.001 h[6]
2.582±0.001 h[6]
5.088±0.004 h[7]
5.154 h[5]
5.191±0.002 h[8]
5.833±0.005 h[9]
0.20 (assumed)[5]
0.232±0.116[3][4]
SMASS = S:[1] · S[5]
15.8[1][5] · 16.1[4]

Numbering and naming edit

This minor planet was numbered by the Minor Planet Center on 23 November 1999.[10] As of 2018, it has not been named.[2]

Orbit and classification edit

1998 OH is a member of the Apollo group of asteroids, which are Earth-crossing asteroids. They are the largest group of near-Earth objects with approximately 10 thousand known members.

It orbits the Sun at a distance of 0.9–2.2 AU in 1 year and 11 months (699 days). Its orbit has an eccentricity of 0.41 and an inclination of 25° with respect to the ecliptic.[1] The body's observation arc begins with a precovery taken at Palomar Observatory in October 1991, more than 7 years prior to its official discovery observation at Haleakala.[2]

Close approaches edit

The asteroid has an Earth minimum orbital intersection distance of 0.0280 AU (4,190,000 km; 2,600,000 mi), which corresponds to 10.9 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size.[1] It will pass close to Earth in 2042 and 2132, at a distance of 0.0292 AU and 0.0317 AU, respectively.[1]

Physical characteristics edit

In the SMASS classification, 1998 OH is a common stony S-type asteroid.[1]

Rotation period edit

In 2014, several rotational lightcurves of 1998 OH were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California, by the Spanish amateur astronomer group OBAS, and by astronomers of the EURONEAR lightcurve NEO survey. Lightcurve analysis gave a rotation period of 5.154 hours with an alternative period solution of 2.58 hours, or half the period. The asteroid's brightness amplitude is rather low with a maximum between 0.11 and 0.20 magnitude, which is indicative for a spherical rather than elongated shape (U=3/3/2-/3/2/2).[5][6][7][8][9][a][b]

Diameter and albedo edit

According to the survey carried out by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, 1998 OH measures 1.663 kilometers in diameter and its surface has an albedo of 0.232.[3][4] The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0.20 and calculates a diameter of 2.06 kilometers based on an absolute magnitude of 15.8.[5]

See also edit

Notes edit

  1. ^ Lightcurve plot of (12538) by Brian Warner (2014) at the Center for Solar System Studies (CS3), with rotation period 5.833±0.005 hours with a brightness amplitude of 0.12±0.02 mag. Quality Code of 2. Summary figures for (12538) at LCDB
  2. ^ Lightcurve plot of (12538) by Brian Warner (2016) at the Center for Solar System Studies (CS3), with rotation period 5.154±0.002 hours with a brightness amplitude of 0.20 mag. Quality Code of 3. Summary figures for (12538) at LCDB

References edit

  1. ^ a b c d e f g h i "JPL Small-Body Database Browser: 12538 (1998 OH)" (2017-09-26 last obs.). Jet Propulsion Laboratory. Retrieved 31 October 2017.
  2. ^ a b c d "12538 (1998 OH)". Minor Planet Center. Retrieved 31 October 2017.
  3. ^ a b c Mainzer, A.; Grav, T.; Bauer, J.; Masiero, J.; McMillan, R. S.; Cutri, R. M.; et al. (December 2011). "NEOWISE Observations of Near-Earth Objects: Preliminary Results". The Astrophysical Journal. 743 (2): 17. arXiv:1109.6400. Bibcode:2011ApJ...743..156M. doi:10.1088/0004-637X/743/2/156.
  4. ^ a b c d Mainzer, A.; Grav, T.; Masiero, J.; Hand, E.; Bauer, J.; Tholen, D.; et al. (November 2011). "NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results". The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90.
  5. ^ a b c d e f g "LCDB Data for (12538)". Asteroid Lightcurve Database (LCDB). Retrieved 31 October 2017.
  6. ^ a b c Vaduvescu, O.; Macias, A. Aznar; Tudor, V.; Predatu, M.; Galád, A.; Gajdos, S.; et al. (August 2017). "The EURONEAR Lightcurve Survey of Near Earth Asteroids". Earth. 120 (2): 41–100. Bibcode:2017EM&P..120...41V. doi:10.1007/s11038-017-9506-9. hdl:10316/80202.
  7. ^ a b Lozano, Juan; Flores, Angel; Mas, Vicente; Fornas, Gonzalo; Rodrigo, Onofre; Brines, Pedro; et al. (April 2017). "Seven Near-Earth Asteroids at Asteroids Observers (OBAS) - MPPD: 2016 June-November". The Minor Planet Bulletin. 44 (2): 108–111. Bibcode:2017MPBu...44..108L. ISSN 1052-8091.
  8. ^ a b Warner, Brian D. (April 2017). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2016 October-December". The Minor Planet Bulletin. 44 (2): 98–107. Bibcode:2017MPBu...44...98W. ISSN 1052-8091.
  9. ^ a b Warner, Brian D. (April 2015). "Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2014 October-December". The Minor Planet Bulletin. 42 (2): 115–127. Bibcode:2015MPBu...42..115W. ISSN 1052-8091.
  10. ^ "MPC/MPO/MPS Archive". Minor Planet Center. Retrieved 24 February 2018.

External links edit

  • at the EARN Near-Earth Asteroids Data Base
  • Asteroid Lightcurve Database (LCDB), query form (info 16 December 2017 at the Wayback Machine)
  • Dictionary of Minor Planet Names, Google books
  • Asteroids and comets rotation curves, CdR – Observatoire de Genève, Raoul Behrend
  • (12538) 1998 OH at NeoDyS-2, Near Earth Objects—Dynamic Site
    • Ephemerides · Observation prediction · Orbital info · MOID · Proper elements · Observational info · Close approaches · Physical info · Orbit animation
  • (12538) 1998 OH at ESA–space situational awareness
    • Ephemerides · Observations · Orbit · Physical properties · Summary
  • (12538) 1998 OH at the JPL Small-Body Database  
    • Close approach · Discovery · Ephemeris · Orbit diagram · Orbital elements · Physical parameters

12538, 1998, stony, asteroid, classified, near, earth, object, potentially, hazardous, asteroid, apollo, group, approximately, kilometers, miles, diameter, discovered, july, 1998, astronomers, near, earth, asteroid, tracking, program, haleakala, observatory, h. 12538 1998 OH is a stony asteroid classified as near Earth object and potentially hazardous asteroid of the Apollo group approximately 1 8 kilometers 1 1 miles in diameter It was discovered on 19 July 1998 by astronomers of the Near Earth Asteroid Tracking program at the Haleakala Observatory in Hawaii United States 2 In 2019 the asteroid came within about 73 lunar distances of Earth 12538 1998 OHDiscovery 1 Discovered byNEATDiscovery siteHaleakala Obs Discovery date19 July 1998DesignationsMPC designation 12538 1998 OHAlternative designations1998 OHMinor planet categoryNEO Apollo PHA 1 2 Orbital characteristics 1 Epoch 4 September 2017 JD 2458000 5 Uncertainty parameter 0Observation arc25 96 yr 9 483 days Aphelion2 1674 AUPerihelion0 9155 AUSemi major axis1 5414 AUEccentricity0 4061Orbital period sidereal 1 91 yr 699 days Mean anomaly58 305 Mean motion0 30m 54s dayInclination24 529 Longitude of ascending node220 75 Argument of perihelion321 72 Earth MOID0 0280 AU 10 9 LDPhysical characteristicsDimensions1 663 0 329 km 3 4 2 06 km calculated 5 Synodic rotation period2 58 0 001 h 6 2 582 0 001 h 6 5 088 0 004 h 7 5 154 h 5 5 191 0 002 h 8 5 833 0 005 h 9 Geometric albedo0 20 assumed 5 0 232 0 116 3 4 Spectral typeSMASS S 1 S 5 Absolute magnitude H 15 8 1 5 16 1 4 Contents 1 Numbering and naming 2 Orbit and classification 3 Close approaches 4 Physical characteristics 4 1 Rotation period 4 2 Diameter and albedo 5 See also 6 Notes 7 References 8 External linksNumbering and naming editThis minor planet was numbered by the Minor Planet Center on 23 November 1999 10 As of 2018 it has not been named 2 Orbit and classification edit1998 OH is a member of the Apollo group of asteroids which are Earth crossing asteroids They are the largest group of near Earth objects with approximately 10 thousand known members It orbits the Sun at a distance of 0 9 2 2 AU in 1 year and 11 months 699 days Its orbit has an eccentricity of 0 41 and an inclination of 25 with respect to the ecliptic 1 The body s observation arc begins with a precovery taken at Palomar Observatory in October 1991 more than 7 years prior to its official discovery observation at Haleakala 2 Close approaches editThe asteroid has an Earth minimum orbital intersection distance of 0 0280 AU 4 190 000 km 2 600 000 mi which corresponds to 10 9 lunar distances and makes it a potentially hazardous asteroid due to its sufficiently large size 1 It will pass close to Earth in 2042 and 2132 at a distance of 0 0292 AU and 0 0317 AU respectively 1 Physical characteristics editIn the SMASS classification 1998 OH is a common stony S type asteroid 1 Rotation period edit In 2014 several rotational lightcurves of 1998 OH were obtained from photometric observations by American astronomer Brian Warner at the Palmer Divide Station in California by the Spanish amateur astronomer group OBAS and by astronomers of the EURONEAR lightcurve NEO survey Lightcurve analysis gave a rotation period of 5 154 hours with an alternative period solution of 2 58 hours or half the period The asteroid s brightness amplitude is rather low with a maximum between 0 11 and 0 20 magnitude which is indicative for a spherical rather than elongated shape U 3 3 2 3 2 2 5 6 7 8 9 a b Diameter and albedo edit According to the survey carried out by the NEOWISE mission of NASA s Wide field Infrared Survey Explorer 1998 OH measures 1 663 kilometers in diameter and its surface has an albedo of 0 232 3 4 The Collaborative Asteroid Lightcurve Link assumes a standard albedo for stony asteroids of 0 20 and calculates a diameter of 2 06 kilometers based on an absolute magnitude of 15 8 5 See also editList of asteroid close approaches to Earth in 2019Notes edit Lightcurve plot of 12538 by Brian Warner 2014 at the Center for Solar System Studies CS3 with rotation period 5 833 0 005 hours with a brightness amplitude of 0 12 0 02 mag Quality Code of 2 Summary figures for 12538 at LCDB Lightcurve plot of 12538 by Brian Warner 2016 at the Center for Solar System Studies CS3 with rotation period 5 154 0 002 hours with a brightness amplitude of 0 20 mag Quality Code of 3 Summary figures for 12538 at LCDBReferences edit a b c d e f g h i JPL Small Body Database Browser 12538 1998 OH 2017 09 26 last obs Jet Propulsion Laboratory Retrieved 31 October 2017 a b c d 12538 1998 OH Minor Planet Center Retrieved 31 October 2017 a b c Mainzer A Grav T Bauer J Masiero J McMillan R S Cutri R M et al December 2011 NEOWISE Observations of Near Earth Objects Preliminary Results The Astrophysical Journal 743 2 17 arXiv 1109 6400 Bibcode 2011ApJ 743 156M doi 10 1088 0004 637X 743 2 156 a b c d Mainzer A Grav T Masiero J Hand E Bauer J Tholen D et al November 2011 NEOWISE Studies of Spectrophotometrically Classified Asteroids Preliminary Results The Astrophysical Journal 741 2 25 arXiv 1109 6407 Bibcode 2011ApJ 741 90M doi 10 1088 0004 637X 741 2 90 a b c d e f g LCDB Data for 12538 Asteroid Lightcurve Database LCDB Retrieved 31 October 2017 a b c Vaduvescu O Macias A Aznar Tudor V Predatu M Galad A Gajdos S et al August 2017 The EURONEAR Lightcurve Survey of Near Earth Asteroids Earth 120 2 41 100 Bibcode 2017EM amp P 120 41V doi 10 1007 s11038 017 9506 9 hdl 10316 80202 a b Lozano Juan Flores Angel Mas Vicente Fornas Gonzalo Rodrigo Onofre Brines Pedro et al April 2017 Seven Near Earth Asteroids at Asteroids Observers OBAS MPPD 2016 June November The Minor Planet Bulletin 44 2 108 111 Bibcode 2017MPBu 44 108L ISSN 1052 8091 a b Warner Brian D April 2017 Near Earth Asteroid Lightcurve Analysis at CS3 Palmer Divide Station 2016 October December The Minor Planet Bulletin 44 2 98 107 Bibcode 2017MPBu 44 98W ISSN 1052 8091 a b Warner Brian D April 2015 Near Earth Asteroid Lightcurve Analysis at CS3 Palmer Divide Station 2014 October December The Minor Planet Bulletin 42 2 115 127 Bibcode 2015MPBu 42 115W ISSN 1052 8091 MPC MPO MPS Archive Minor Planet Center Retrieved 24 February 2018 External links edit 12538 1998 OH at the EARN Near Earth Asteroids Data Base Asteroid Lightcurve Database LCDB query form info Archived 16 December 2017 at the Wayback Machine Dictionary of Minor Planet Names Google books Asteroids and comets rotation curves CdR Observatoire de Geneve Raoul Behrend 12538 1998 OH at NeoDyS 2 Near Earth Objects Dynamic Site Ephemerides Observation prediction Orbital info MOID Proper elements Observational info Close approaches Physical info Orbit animation 12538 1998 OH at ESA space situational awareness Ephemerides Observations Orbit Physical properties Summary 12538 1998 OH 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 12538 1998 OH amp oldid 1198064408, wikipedia, wiki, book, books, library,

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