(5645) 1990 SP

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(5645) 1990 SP
Discovery [1]
Discovered by R. H. McNaught
Discovery site Siding Spring Obs.
Discovery date 20 September 1990
MPC designation (5645) 1990 SP
1990 SP
Apollo · NEO[2]
Orbital characteristics[1]
Epoch 31 July 2016 (JD 2457600.5)
Uncertainty parameter 0
Observation arc 40.89 yr (14,935 days)
Aphelion 1.8797 AU
Perihelion 0.8302 AU
1.3549 AU
Eccentricity 0.3873
1.58 yr (576 days)
0° 37m 29.64s / day
Inclination 13.507°
Earth MOID 0.0546 AU
Physical characteristics
Dimensions 1.648 km[3]
1.65 km (taken)[4]
1.668±0.018 km[5]
1.849±0.334 km[6]
2.20±0.74 km[7]
30.39±0.04 h[8]
P[9] · CXT[10] · S[4]
16.75±0.2 (R)[8]

(5645) 1990 SP is an eccentric and tumbling asteroid, classified as near-Earth object and Apollo asteroid, approximately 1.7 kilometers in diameter. It was discovered on 20 September 1990, by Scottish–Australian astronomer Robert McNaught at the Siding Spring Observatory in Canberra, Australia.[2]

The asteroid orbits the Sun at a distance of 0.8–1.9 AU once every 1 years and 7 months (576 days). Its orbit has an eccentricity of 0.39 and an inclination of 14° with respect to the ecliptic.[1] The first precovery was taken at the discovering observatory during the Digital Sky Survey (DSS) in 1974, extending the asteroid's observation arc by 16 years prior to its discovery.[2] This near-Earth asteroid has an Earth minimum orbit intersection distance of 0.055 AU (8,200,000 km), only slightly above the threshold minimum distance of 19.5 lunar distances (0.05 AU) to make it a potentially hazardous object. It also makes close approaches to Mars. On 14 April 1969, it passed the Red Planet at only 0.013 AU (1,900,000 km).[1]

The stony S-type asteroid is also classified as a P-type asteroid, based on post-cryogenic observations by the Spitzer Space Telescope,[9] while observations at the NASA Infrared Telescope Facility using its SpeX instrument during a follow-up campaign of the Spitzer-observed objects between 2009 and 2012, gave it a C/X/T spectral type.[10]

In April 2002, Czech astronomer Petr Pravec obtained a rotational light-curve from a photometric observations, which gave a relatively long period of 30.39±0.04 hours with a brightness variation of 0.7 in magnitude (U=2). The observations have also shown that the body is most likely in a tumbling motion.[4][8]

Estimates for the body's diameter range from 1.6 to 2.2 kilometers with an albedo for its surface between 0.06 and 0.12, according to observations made by the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer and by the Spitzer Space Telescope.[3][5][6][7] The Collaborative Asteroid Lightcurve Link takes the revised WISE data – an albedo of 0.0872 and a diameter of 1.65 kilometers – as the best of all available results.[3][4]


  1. ^ a b c d e "JPL Small-Body Database Browser: 5645 (1990 SP)" (2015-07-04 last obs.). Jet Propulsion Laboratory. Retrieved 29 June 2016. 
  2. ^ a b c "5645 (1990 SP)". Minor Planet Center. Retrieved 29 June 2016. 
  3. ^ a b c d e Pravec, Petr; Harris, Alan W.; Kusnirák, Peter; Galád, Adrián; Hornoch, Kamil (September 2012). "Absolute magnitudes of asteroids and a revision of asteroid albedo estimates from WISE thermal observations". Icarus. 221 (1): 365–387. Bibcode:2012Icar..221..365P. doi:10.1016/j.icarus.2012.07.026. Retrieved 29 June 2016. 
  4. ^ a b c d e "LCDB Data for (5645)". Asteroid Lightcurve Database (LCDB). Retrieved 29 June 2016. 
  5. ^ 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" (PDF). The Astrophysical Journal. 741 (2): 25. arXiv:1109.6407free to read. Bibcode:2011ApJ...741...90M. doi:10.1088/0004-637X/741/2/90. Retrieved 29 June 2016. 
  6. ^ a b c d Mainzer, 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. Bibcode:2012ApJ...760L..12M. doi:10.1088/2041-8205/760/1/L12. Retrieved 29 June 2016. 
  7. ^ a b c Mueller, 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. Retrieved 29 June 2016. 
  8. ^ a b c Pravec, P.; Harris, A. W.; Scheirich, P.; Kusnirák, P.; Sarounová, L.; Hergenrother, C. W.; et al. (January 2005). "Tumbling asteroids". Icarus. 173 (1): 108–131. Bibcode:2005Icar..173..108P. doi:10.1016/j.icarus.2004.07.021. Retrieved 29 June 2016. 
  9. ^ a b c 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. Retrieved 29 June 2016. 
  10. ^ a b 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:1310.2000free to read. Bibcode:2014Icar..228..217T. doi:10.1016/j.icarus.2013.10.004. Retrieved 29 June 2016. 

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