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(10115) 1992 SK

From Wikipedia, the free encyclopedia
Apollo minor planet, NEO and PHA

(10115) 1992 SK
Discovery[1]
Discovered byE. F. Helin
J. Alu
Discovery sitePalomar Obs.
Discovery date24 September 1992
Designations
(10115) 1992 SK
1992 SK · 1985 SD
1985 TO2
Apollo · NEO · PHA[1][2]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc63.57 yr (23,219 days)
Aphelion1.6539AU
Perihelion0.8429 AU
1.2484 AU
Eccentricity0.3248
1.39yr (509 days)
47.505°
0° 42m 23.76s / day
Inclination15.322°
8.9232°
233.63°
Earth MOID0.0449 AU · 17.5LD
Physical characteristics
0.90±0.20 km[3]
0.938±0.294 km[4]
1.000±0.085 km[5]
1.0±0.2[6]
1.18 km(calculated)[7]
7.31±0.02 h[8]
7.31832 h[9]
7.319 h[7]
7.323±0.005 h[10]
7.328±0.002h[a]
7.320232±0.000010 h[6]
0.20(assumed)[7]
0.2799±0.1397[5]
0.318±0.214[4]
0.34±0.25[3]
0.38±0.24[11]
SMASS =S[1] · S[7] · S/Sq[12]
17.0[1][4][5][7] · 17.4[a]

(10115) 1992 SK, is a stonynear-Earth object andpotentially hazardous asteroid on an eccentric orbit. It belongs to the group ofApollo asteroids and measures approximately 1 kilometer (0.6 miles) in diameter. It was discovered by American astronomersEleanor Helin andJeff Alu at thePalomar Observatory in California on 24 September 1992.[2]

Classification and orbit

[edit]

The asteroid orbits the Sun at a distance of 0.8–1.7 AU once every 17 months (509 days). Its orbit has aneccentricity of 0.32 and aninclination of 15° with respect to theecliptic. Its Earthminimum orbit intersection distance is 0.0449 AU (6,720,000 km). This makes the body a potentially hazardous asteroid, because itsMOID is less than 0.05 AU and its diameter is greater than 150 meters.[1] The firstprecovery was obtained at Palomar Observatory in 1953, extending the asteroid'sobservation arc by 39 years prior to its discovery.[2]

Physical characteristics

[edit]

In theSMASS classification,1992 SK is characterized as a common stonyS-type asteroid.[1]

Rotation period

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Several rotationallightcurves form photometric observations have been obtained for this body. In 1999, Czech astronomerPetr Pravec constructed a lightcurve, that rendered arotation period of7.328 hours and a brightness variation of 0.72 inmagnitude (U=n/a).[a]

In March 2006, observations by astronomer David Polishook from the ground-basedWise Observatory, Israel, gave a rotation period of7.31 and amplitude of 0.70 mag (U=2),[8] and in November 2011, American astronomerBrian Warner at the Palmer Divide Observatory, Colorado, obtained the first well-defined period of7.323 hours with an amplitude of 0.50 mag (U=3).[10]

The rotation period of 1992 SK is slowly accelerating due to theYORP effect.[6]

Diameter and albedo

[edit]

According to the surveys carried out by NASA's space-basedWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures 1.0 and 0.94 kilometers in diameter and its surface has analbedo of 0.28 to 0.32, respectively.[4][5] The ExploreNEOs project finds an albedo of 0.34, with a diameter of 0.9 kilometers,[3] and theCollaborative Asteroid Lightcurve Link calculates a diameter of 1.18 kilometers based on an assumed standard albedo for stony asteroids of 0.20 and anabsolute magnitude of 17.0.[7]

Numbering and naming

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Thisminor planet wasnumbered by theMinor Planet Center on 2 March 1999.[13] As of 2019[update], it has not beennamed.[2]

Notes

[edit]
  1. ^abcPravec (1999) web: rotation period7.328±0.002 hours with a brightness amplitude of0.72 mag. Two more light-curves rendered similar periods. No quality rating by CALL. Summary figures atCollaborative Asteroid Lightcurve Link (CALL) for (10115)

References

[edit]
  1. ^abcdefg"JPL Small-Body Database Browser: 10115 (1992 SK)" (2017-05-08 last obs.).Jet Propulsion Laboratory. Retrieved26 May 2017.
  2. ^abcd"10115 (1992 SK)".Minor Planet Center. Retrieved1 April 2016.
  3. ^abcMueller, Michael; Delbo', M.; Hora, J. L.; Trilling, D. E.; Bhattacharya, B.; Bottke, W. F.; et al. (April 2011)."ExploreNEOs. III. Physical Characterization of 65 Potential Spacecraft Target Asteroids".The Astronomical Journal.141 (4): 9.Bibcode:2011AJ....141..109M.doi:10.1088/0004-6256/141/4/109.S2CID 44827674. Retrieved1 April 2016.
  4. ^abcdMainzer, A.; Grav, T.; Masiero, J.; Bauer, J.; Cutri, R. M.; McMillan, R. S.; et al. (November 2012)."Physical Parameters of Asteroids Estimated from the WISE 3-Band Data and NEOWISE Post-Cryogenic Survey".The Astrophysical Journal Letters.760 (1): 6.arXiv:1210.0502.Bibcode:2012ApJ...760L..12M.doi:10.1088/2041-8205/760/1/L12.S2CID 41459166. Retrieved1 April 2016.
  5. ^abcdMainzer, 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.S2CID 35447010. Retrieved1 April 2016.
  6. ^abcĎurech, J.; et al. (2022). "Rotation acceleration of asteroids (10115) 1992 SK, (1685) Toro, and (1620) Geographos due to the YORP effect".Astronomy & Astrophysics.657: A5.arXiv:2110.06548.Bibcode:2022A&A...657A...5D.doi:10.1051/0004-6361/202141844.S2CID 238744034.
  7. ^abcdef"LCDB Data for (10115)". Asteroid Lightcurve Database (LCDB). Retrieved1 April 2016.
  8. ^abPolishook, David (July 2012)."Lightcurves and Spin Periods of Near-Earth Asteroids, The Wise Observatory, 2005 - 2010".The Minor Planet Bulletin.39 (3):187–192.Bibcode:2012MPBu...39..187P.ISSN 1052-8091. Retrieved1 April 2016.
  9. ^Busch, Michael W.; Ostro, Steven J.; Benner, Lance A. M.; Giorgini, Jon D.; Jurgens, Raymond F.; Rose, Randy; et al. (March 2006)."Radar and optical observations and physical modeling of near-Earth Asteroid 10115 (1992 SK)".Icarus.181 (1):145–155.Bibcode:2006Icar..181..145B.doi:10.1016/j.icarus.2005.10.024. Retrieved1 April 2016.
  10. ^abWarner, Brian D. (April 2014)."Near-Earth Asteroid Lightcurve Analysis at CS3-Palmer Divide Station: 2013 September–December".The Minor Planet Bulletin.41 (2):113–124.Bibcode:2014MPBu...41..113W.ISSN 1052-8091.PMC 7268210.PMID 32494788. Retrieved1 April 2016.
  11. ^Thomas, C. A.; Trilling, D. E.; Emery, J. P.; Mueller, M.; Hora, J. L.; Benner, L. A. M.; et al. (September 2011)."ExploreNEOs. V. Average Albedo by Taxonomic Complex in the Near-Earth Asteroid Population".The Astronomical Journal.142 (3): 12.Bibcode:2011AJ....142...85T.doi:10.1088/0004-6256/142/3/85.
  12. ^Thomas, Cristina A.; Emery, Joshua P.; Trilling, David E.; Delbó, Marco; Hora, Joseph L.; Mueller, Michael (January 2014)."Physical characterization of Warm Spitzer-observed near-Earth objects".Icarus.228:217–246.arXiv:1310.2000.Bibcode:2014Icar..228..217T.doi:10.1016/j.icarus.2013.10.004.hdl:2060/20140012047.S2CID 119278697. Retrieved1 April 2016.
  13. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved24 February 2018.

External links

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