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2228 Soyuz-Apollo

From Wikipedia, the free encyclopedia
Main-belt asteroid

2228 Soyuz–Apollo
Discovery[1]
Discovered byN. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date19 July 1977
Designations
(2228) Soyuz–Apollo
Named after
Apollo–Soyuz(Test Project)[2]
1977 OH · 1933 SK1
1952 DT1 · 1963 DD
1973 YN3
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc53.75 yr (19,632 days)
Aphelion3.7135AU
Perihelion2.5605 AU
3.1370 AU
Eccentricity0.1838
5.56yr (2,029 days)
341.70°
0° 10m 38.64s / day
Inclination1.9888°
140.40°
285.71°
Physical characteristics
Dimensions23.55 km(calculated)[3]
26.080±0.295 km[4][5]
28.26±0.49 km[6]
5.3846±0.0007 h[7]
5.3868±0.0013 h[8]
5.4±0.05 h[7]
6.12h[9]
0.08(assumed)[3]
0.101±0.004[6]
0.113±0.020[5]
0.1134±0.0198[4]
C[3]
10.9[4][6] · 11.21±0.42[10] · 11.5[1][3] · 11.848±0.002(S)[8]

2228 Soyuz–Apollo, provisional designation1977 OH, is a carbonaceousThemistian asteroid from the outer region of theasteroid belt, approximately 26 kilometers in diameter. It was discovered on 19 July 1977, by Soviet–Russian astronomerNikolai Chernykh at theCrimean Astrophysical Observatory in Nauchnyj on the Crimean peninsula.[11] It was named after theApollo–Soyuz Test Project.[2]

Orbit and classification

[edit]

The darkC-type asteroid is a member of theThemis family, a dynamical family of outer-belt asteroids with nearly coplanarecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.6–3.7 AU once every 5 years and 7 months (2,029 days). Its orbit has aneccentricity of 0.18 and aninclination of 2° with respect to theecliptic.[1]

Physical characteristics

[edit]

It has arotation period of 5.4 hours and analbedo of 0.10 and 0.11, as determined by the space-basedAkari andWISE missions, respectively,[6][4] while the Collaborative Asteroid Lightcurve Link (CALL) assumes a lower albedo of 0.08.[3]

Naming

[edit]

Thisminor planet was named after the joint Soviet-American space flight, theApollo–Soyuz Test Project, carried on in 1975. The reversal of the names, "Soyuz–Apollo" rather than "Apollo–Soyuz", was not political, but to prevent confusion with the asteroid1862 Apollo.[2] The official naming citation was published by theMinor Planet Center on 1 March 1981 (M.P.C. 5850).[12]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2228 Soyuz–Apollo (1977 OH)" (2016-11-23 last obs.).Jet Propulsion Laboratory. Retrieved12 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2228) Soyuz–Apollo".Dictionary of Minor Planet Names – (2228) Soyuz–Apollo.Springer Berlin Heidelberg. p. 181.doi:10.1007/978-3-540-29925-7_2229.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2228) Soyuz–Apollo". Asteroid Lightcurve Database (LCDB). Retrieved7 December 2016.
  4. ^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.
  5. ^abMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Dailey, J.; et al. (November 2011)."Main Belt Asteroids with WISE/NEOWISE. I. Preliminary Albedos and Diameters".The Astrophysical Journal.741 (2): 20.arXiv:1109.4096.Bibcode:2011ApJ...741...68M.doi:10.1088/0004-637X/741/2/68.S2CID 118745497. Retrieved7 December 2016.
  6. ^abcdUsui, Fumihiko; Kuroda, Daisuke; Müller, Thomas G.; Hasegawa, Sunao; Ishiguro, Masateru; Ootsubo, Takafumi; et al. (October 2011). "Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey".Publications of the Astronomical Society of Japan.63 (5):1117–1138.Bibcode:2011PASJ...63.1117U.doi:10.1093/pasj/63.5.1117. (online,AcuA catalog p. 153)
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2228) Soyuz–Apollo".Geneva Observatory. Retrieved7 December 2016.
  8. ^abWaszczak, Adam; Chang, Chan-Kao; Ofek, Eran O.; Laher, Russ; Masci, Frank; Levitan, David; et al. (September 2015)."Asteroid Light Curves from the Palomar Transient Factory Survey: Rotation Periods and Phase Functions from Sparse Photometry".The Astronomical Journal.150 (3): 35.arXiv:1504.04041.Bibcode:2015AJ....150...75W.doi:10.1088/0004-6256/150/3/75.S2CID 8342929. Retrieved7 December 2016.
  9. ^Almeida, R.; Angeli, C. A.; Duffard, R.; Lazzaro, D. (February 2004)."Rotation periods for small main-belt asteroids".Astronomy and Astrophysics.415:403–406.Bibcode:2004A&A...415..403A.doi:10.1051/0004-6361:20034585.
  10. ^Veres, Peter; Jedicke, Robert; Fitzsimmons, Alan; Denneau, Larry; Granvik, Mikael; Bolin, Bryce; et al. (November 2015)."Absolute magnitudes and slope parameters for 250,000 asteroids observed by Pan-STARRS PS1 - Preliminary results".Icarus.261:34–47.arXiv:1506.00762.Bibcode:2015Icar..261...34V.doi:10.1016/j.icarus.2015.08.007.S2CID 53493339. Retrieved7 December 2016.
  11. ^"2228 Soyuz–Apollo (1977 OH)".Minor Planet Center. Retrieved7 December 2016.
  12. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved7 December 2016.

External links

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