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2085 Henan

From Wikipedia, the free encyclopedia
Asteroid

2085 Henan
Discovery[1]
Discovered byPurple Mountain Obs.
Discovery sitePurple Mountain Obs.
Discovery date20 December 1965
Designations
(2085) Henan
Named after
Henan(Province of China)[2]
1965 YA · 1933 RE
1938 WR · 1949 FL
1949 FP1 · 1962 CL
1963 KA · 1969 VA1
1971 BG1 · 1972 LX
1973 QX1 · 1976 GR7
main-belt · (outer)
Henan[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc68.61 yr (25,060 days)
Aphelion2.9312AU
Perihelion2.4654 AU
2.6983 AU
Eccentricity0.0863
4.43yr (1,619 days)
276.34°
0° 13m 20.64s / day
Inclination3.8343°
118.14°
294.54°
Physical characteristics
Dimensions13.356±0.036 km[4]
13.67 km(calculated)[5]
13.941±0.082 km[6]
16.56±4.50 km[7]
17.61±0.32 km[8]
18 km[9]: 23 
18.34±1.20 km[10]
24h[11]
110±1 h[12]
0.10±0.08[7]
0.131±0.019[8]
0.145±0.020[10]
0.18(assumed)[5]
0.2510±0.0408[6]
SMASS =L[1][5]
L(Bus–DeMeo)[12]
11.40[6][10] · 11.55±0.48[13] · 11.60[8] · 11.8[5] · 11.9[1] · 12.12[7]

2085 Henan, provisional designation1965 YA, is a potentially slow rotatingasteroid and the parent body of theHenan family in the central regions of theasteroid belt, approximately 15 kilometers in diameter. It was discovered on 20 December 1965, by astronomers at thePurple Mountain Observatory in Nanking, China.[14] The asteroid was named for theHenan Province in China.[2]

Orbit and classification

[edit]

Henan is theparent body of theHenan family (532),[3] a largefamily ofL-type asteroids in the intermediate main-belt, which can be further divided into four distinct families.[9]: 23 

It orbits the Sun in thecentral asteroid belt at a distance of 2.5–2.9 AU once every 4 years and 5 months (1,619 days;semi-major axis of 2.70 AU). Its orbit has aneccentricity of 0.09 and aninclination of 4° with respect to theecliptic.[1]

A first observation of this asteroid was found on aprecovery, taken at theLowell Observatory in July 1906. The body'sobservation arc begins atGoethe Link Observatory in July 1943, more than 22 years prior to its official discovery observation at Purple Mountain.[14]

Physical characteristics

[edit]

In the Bus–DeMeo andSMASS classification,Henan is an uncommonL-type asteroid,[1][5][12]: 5  which is also the overallspectral type for members of theHenan family.[9]: 23 

Rotation period

[edit]

As of 2017, no secure rotationallightcurve ofHenan has been obtained. In September 2004, observations byLaurent Bernasconi gave arotation period of 24 hours with a brightness variation of 0.25magnitude (U=1).[11] In February 2015, photometric observations ofHenan by an international collaboration of astronomers gave a tentative synodic period of110±1 hours and an amplitude of 0.4 magnitude, which would make it a potentiallyslow rotator (U=1).[12] An alternative period solution gave 94 hours. The latter study selectedHenan because it is a suspected "Barbarian" asteroid (named after234 Barbara) which polarimetric properties suggest that they have an unusual shape and topographic features with large concave areas.[12]

Diameter and albedo

[edit]

According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Henan measures between 13.356 and 18.34 kilometers in diameter and its surface has analbedo between 0.10 and 0.2510.[4][6][7][8][10]

TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.18 and calculates a diameter of 13.67 kilometers based on anabsolute magnitude of 11.8.[5]

Naming

[edit]

Thisminor planet was named after theHenan Province in the People's Republic of China, located in the central part of the country along the lower stretch of theYellow River, which is considered the cradle of civilization in ancient China.[2] The official naming citation was published by theMinor Planet Center on 1 February 1980 (M.P.C. 5184).[15]

References

[edit]
  1. ^abcdef"JPL Small-Body Database Browser: 2085 Henan (1965 YA)" (2017-11-02 last obs.).Jet Propulsion Laboratory. Retrieved18 November 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2085) Henan".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 169.doi:10.1007/978-3-540-29925-7_2086.ISBN 978-3-540-00238-3.
  3. ^ab"Asteroid 2085 Henan – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  4. ^abMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014). "Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121.
  5. ^abcdef"LCDB Data for (2085) Henan". Asteroid Lightcurve Database (LCDB). Retrieved18 November 2017.
  6. ^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.
  7. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  8. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved18 November 2017.
  9. ^abcNesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  10. ^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)
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2085) Henan". Geneva Observatory. Retrieved18 November 2017.
  12. ^abcdeDevogè; le, M.; Tanga, P.; Bendjoya, P.; Rivet, J. P.; Surdej, J.; et al. (July 2017). "Shape and spin determination of Barbarian asteroids".Astronomy & Astrophysics.607 (119): A119.arXiv:1707.07503.Bibcode:2017A&A...607A.119D.doi:10.1051/0004-6361/201630104.
  13. ^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. Retrieved18 November 2017.
  14. ^ab"2085 Henan (1965 YA)".Minor Planet Center. Retrieved18 November 2017.
  15. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved18 November 2017.


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