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1772 Gagarin

From Wikipedia, the free encyclopedia
Main-belt asteroid
This article is about the asteroid. For the lunar crater, seeGagarin (crater).

1772 Gagarin
Shape model ofGagarin from itslightcurve
Discovery[1]
Discovered byL. Chernykh
Discovery siteCrimean Astrophysical Obs.
Discovery date6 February 1968
Designations
(1772) Gagarin
Named after
Yuri Gagarin(cosmonaut)[2]
1968 CB · 1940 GA
1942 VZ · 1948 ET
1960 FH · 1969 OO
main-belt · (middle)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc76.21 yr (27,835 days)
Aphelion2.7924AU
Perihelion2.2610 AU
2.5267 AU
Eccentricity0.1051
4.02yr (1,467 days)
90.345°
0° 14m 43.44s / day
Inclination5.7423°
88.181°
93.442°
Physical characteristics
Dimensions8.00 km(derived)[3]
8.838±0.644[4]
9.634±0.105 km[5]
10.93791±0.00005 h[6]
10.94130±0.00005 h[7]
10.9430±0.0049 h[8]
10.96h[9]
0.1380±0.0085[5]
0.164±0.039[4]
0.20(assumed)[3]
L[10] · S[3]
B–V = 0.920[1]
12.626±0.002(R)[8] · 12.7[1] · 12.80±0.45[10] · 12.85[3][9][5]

1772 Gagarin (prov. designation:1968 CB) is a stonybackground asteroid from the central region of theasteroid belt, approximately 9 kilometers in diameter. It was discovered on 6 February 1968, by Russian astronomerLyudmila Chernykh at theCrimean Astrophysical Observatory in Nauchnyj, on the Crimean Peninsula.[11] The asteroid was named after cosmonautYuri Gagarin.[2]

Orbit and classification

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Gagarin orbits the Sun in thecentral main-belt at a distance of 2.3–2.8 AU once every 4.02 years (1,467 days). Its orbit has aneccentricity of 0.11 and aninclination of 6° with respect to theecliptic.[1]Gagarin first observation is aprecovery that was taken atTurku Observatory in 1940, extending the body'sobservation arc by 28 years prior to its official discovery observation.[11]

Physical characteristics

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Gagarin has been characterized as a rareL-type asteroid byPanSTARRS' photometric survey.[10]

Rotation period

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In February 1984, a rotationallightcurve ofGagarin obtained by American astronomerRichard P. Binzel gave arotation period of 10.96 hours with a brightness variation of 0.24magnitude (U=2).[9] Photometric observations at the CalifornianPalomar Transient Factory in December 2011, gave a 10.9430 hours with an amplitude of 0.41 (U=2).[8] in 2001 and 2016, additional lightcurve were obtained from modeled photometric data, giving a period of 10.94130 and 10.93791 hours (U=n.a.).[6][7]

Diameter and albedo

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According to the survey carried out by NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Gagarin measures between 8.83 and 9.63 kilometers in diameter, and its surface has analbedo between 0.138 and 0.164,[4][5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo of 0.20 and derives a diameter of 8.00 kilometers with anabsolute magnitude of 12.85.[3]

Naming

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Thisminor planet was named for Russian–Soviet cosmonautYuri Gagarin (1934–1968),Hero of the Soviet Union and first human to journey into outer space by circumnavigating Earth in 1961. Gagarin died in a jet fighter crash in 1968, the year the asteroid was discovered. The lunar craterGagarin is also named in his honor.[2] The officialnaming citation was published by theMinor Planet Center on 25 September 1971 (M.P.C. 3185).[12]

See also

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References

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  1. ^abcde"JPL Small-Body Database Browser: 1772 Gagarin (1968 CB)" (2016-06-16 last obs.).Jet Propulsion Laboratory. Retrieved8 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1772) Gagarin".Dictionary of Minor Planet Names – (1772) Gagarin.Springer Berlin Heidelberg. p. 142.doi:10.1007/978-3-540-29925-7_1773.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1772) Gagarin". Asteroid Lightcurve Database (LCDB). Retrieved20 December 2016.
  4. ^abcMasiero, 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. Retrieved20 December 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.
  6. ^abHanus, J.; Durech, J.; Oszkiewicz, D. A.; Behrend, R.; Carry, B.; Delbo, M.; et al. (February 2016)."New and updated convex shape models of asteroids based on optical data from a large collaboration network".Astronomy and Astrophysics.586: 24.arXiv:1510.07422.Bibcode:2016A&A...586A.108H.doi:10.1051/0004-6361/201527441. Retrieved20 December 2016.
  7. ^abHanus, J.; Durech, J.; Broz, M.; Warner, B. D.; Pilcher, F.; Stephens, R.; et al. (June 2011)."A study of asteroid pole-latitude distribution based on an extended set of shape models derived by the lightcurve inversion method".Astronomy & Astrophysics.530: 16.arXiv:1104.4114.Bibcode:2011A&A...530A.134H.doi:10.1051/0004-6361/201116738. Retrieved20 December 2016.
  8. ^abcWaszczak, 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. Retrieved20 December 2016.
  9. ^abcBinzel, R. P. (October 1987)."A photoelectric survey of 130 asteroids".Icarus.72 (1):135–208.Bibcode:1987Icar...72..135B.doi:10.1016/0019-1035(87)90125-4.ISSN 0019-1035. Retrieved20 December 2016.
  10. ^abcVeres, 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. Retrieved20 December 2016.
  11. ^ab"1772 Gagarin (1968 CB)".Minor Planet Center. Retrieved20 December 2016.
  12. ^Schmadel, Lutz D. (2009). "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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