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1897 Hind

From Wikipedia, the free encyclopedia
Asteroid

1897 Hind
Discovery[1]
Discovered byL. Kohoutek
Discovery siteBergedorf Obs.
Discovery date26 October 1971
Designations
(1897) Hind
Named after
John Russell Hind
(English astronomer)[2]
1971 UE1 · 1957 SG
main-belt · Flora[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc61.03 yr (22,291 days)
Aphelion2.6088AU
Perihelion1.9565 AU
2.2826 AU
Eccentricity0.1429
3.45yr (1,260 days)
155.47°
0° 17m 8.88s / day
Inclination4.0545°
63.423°
269.03°
Physical characteristics
Dimensions5.007±0.103 km[4][5]
5.67 km(calculated)[3]
0.82±0.01h[6]
2.6336±0.0001 h[7]
0.24(assumed)[3]
0.307±0.024[5]
0.3075±0.0240[4]
S[3]
13.4[1][3][4] · 13.81±0.72[8]

1897 Hind, provisional designation1971 UE1, is a Florianasteroid from the inner regions of theasteroid belt, approximately 5 kilometers in diameter. It was discovered on 26 October 1971, by Czech astronomerLuboš Kohoutek atBergedorf Observatory in Hamburg, Germany.[9] The asteroid was named after English astronomerJohn Russell Hind.[2]

Orbit and classification

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Hind is a member of theFlora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in theinner main-belt at a distance of 2.0–2.6 AU once every 3 years and 5 months (1,260 days). Its orbit has aneccentricity of 0.14 and aninclination of 4° with respect to theecliptic.[1]

A firstprecovery was taken atPalomar Observatory in 1956, extending the asteroid'sobservation arc by 15 years prior to its discovery.[9]

Physical characteristics

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Hind has been characterized as a stonyS-type asteroid.[3]

Diameter and albedo

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According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Hind measures 5.0 kilometers in diameter and its surface has analbedo of 0.307,[4][5] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo of 0.24 – derived from8 Flora, the family's largest member and namesake – and calculates a diameter of 5.7 kilometers with anabsolute magnitude of 13.4.[3]

Rotation period

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In July 2005,Hind had originally been identified as a relativelyfast rotator, as photometric observations by astronomersReiner Stoss,Jaime Nomen,Salvador Sanchez andRaoul Behrend gave arotation period of0.82±0.01 hours, or less than 50 minutes (U=1).[6] However, the lightcurve was only fragmentary. In August 2012, it was superseded with more accurate observation at the Australian Riverland Dingo Observatory that gave a slower period of2.6336±0.0001 hours with a brightness variation of 0.09 inmagnitude (U=2).[7]

Naming

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Thisminor planet was named after English astronomerJohn Russell Hind (1823–1895),discoverer of ten minor planets including7 Iris and8 Flora, the namesake of the family the asteroid belongs to. Hind worked for many years atGeorge Bishop's Observatory near London where he made his discoveries. He was also superintendent of the BritishNautical Almanac Office in the second half of the 19th century.[2] The officialnaming citation was published by theMinor Planet Center on 1 June 1975 (M.P.C. 3827).[10]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1897 Hind (1971 UE1)" (2017-03-27 last obs.).Jet Propulsion Laboratory. Retrieved9 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1897) Hind".Dictionary of Minor Planet Names – (1897) Hind.Springer Berlin Heidelberg. p. 152.doi:10.1007/978-3-540-29925-7_1898.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (1897) Hind". Asteroid Lightcurve Database (LCDB). Retrieved23 August 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.
  5. ^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. Retrieved8 December 2016.
  6. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1897) Hind".Geneva Observatory. Retrieved23 August 2016.
  7. ^abHills, Kevin (January 2013)."Asteroid Lightcurve Analysis at Riverland Dingo Observatory (RDO): 501 Urhixidur, 1897 Hind, 1928 Summa, 6261 Chione, and (68216) 2001 CV 26".The Minor Planet Bulletin.40 (1):12–13.Bibcode:2013MPBu...40...12H.ISSN 1052-8091. Retrieved23 August 2016.
  8. ^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. Retrieved23 August 2016.
  9. ^ab"1897 Hind (1971 UE1)".Minor Planet Center. Retrieved23 August 2016.
  10. ^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

[edit]
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Authority control databasesEdit this at Wikidata
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