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2000 Herschel

From Wikipedia, the free encyclopedia
Main-belt asteroid

2000 Herschel
Discovery[1]
Discovered byJ. Schubart
Discovery siteSonneberg Obs.
Discovery date29 July 1960
Designations
(2000) Herschel
Pronunciation/ˈhɜːrʃəl/[2]
Named after
William Herschel[3]
(German-British astronomer)
1960 OA · 1934 NX
main-belt[1][4] · (inner)[5]
Phocaea[6]
Orbital characteristics[4]
Epoch 27 April 2019 (JD 2458600.5)
Uncertainty parameter 0
Observation arc84.08yr (30,712 d)
Aphelion3.0885AU
Perihelion1.6708 AU
2.3796 AU
Eccentricity0.2979
3.67 yr (1,341 d)
293.69°
0° 16m 6.6s / day
Inclination22.819°
291.92°
130.51°
Physical characteristics
14.768±0.348 km[7][8]
16.15±3.11 km[9]
16.86±1.17 km[10]
17.385±0.173 km[11]
130±h[5][12]
0.1870[11]
0.197[10]
0.24[9]
0.256[7][8]
Tholen =S[4][5]
B–V = 0.893[4]
U–B = 0.494[4]
11.25[1][4][5][7][10][11]
11.42[9]

2000 Herschel, provisional designation1960 OA, is a stony Phocaeaasteroid and a tumblingslow rotator from the inner regions of theasteroid belt, approximately 16 kilometers (10 miles) in diameter. It was discovered 29 July 1960, by German astronomerJoachim Schubart atSonneberg Observatory in eastern Germany.[1] TheS-type asteroid has a longrotation period of 130 hours.[5] It was named after astronomerWilliam Herschel.[3]

Orbit and classification

[edit]

Herschel is a member of thePhocaea family (701),[6] a largefamily of stony asteroids with nearly two thousand known members.[13]: 23  It orbits the Sun in theinner main-belt at a distance of 1.7–3.1 AU once every 3 years and 8 months (1,341 days;semi-major axis of 2.38 AU). Its orbit has aneccentricity of 0.30 and aninclination of 23° with respect to theecliptic.[4] It was first identified as1934 NX atJohannesburg Observatory in 1934, extending the body'sobservation arc by 26 years prior to its official discovery observation at Sonneberg.[1]

The relatively highorbital eccentricity of this object causes it to come close to the orbit of the planetMars. This means there is a chance it will eventually collide with the planet, with the odds of a collision estimated at 18% per billion orbits.[14]

Naming

[edit]

Thisminor planet was named in honour of the English astronomer of German originWilliam Herschel (1738–1822), who discovered what he calledGeorgium Sidus (akaUranus). The officialnaming citation was published by theMinor Planet Center on 15 October 1977 (M.P.C. 4237).[15] While the minor planet with number "1000",1000 Piazzia, honors the discoverer of the first minor planet,Giuseppe Piazzi, number "2000" does so for Herschel, discoverer of the first telescopic major planet.[3] The asteroid is one of several early "kilo-numbered" minor planets that were dedicated to renowned scientists or institutions including:[16]

The sequence continues with the asteroids5000 IAU (for theInternational Astronomical Union),6000 United Nations (for theUnited Nations),7000 Curie (for the pioneers on radioactivity,Marie andPierre Curie), and8000 Isaac Newton (forIsaac Newton),[16] while9000 Hal (afterHAL 9000 from2001: A Space Odyssey) and10000 Myriostos (after the Greek word for ten-thousandth, which is meant to honor all astronomers) were named based on their direct numeric accordance.

Physical characteristics

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In theTholen classification,Herschel is a commonS-type asteroid.[4]

Slow rotator and tumbler

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Analysis of thelightcurve for this object appears to show that it istumbling, with rotation occurring about the non-principal axis. Lightcurve analysis gave arotation period of130±3 hours with a high brightness variation of1.16±0.05magnitude (U=2).[12] This makes it aslow rotator.[5]

Diameter and albedo

[edit]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroid of 0.20 and calculates a diameter of 16.71 kilometers based on anabsolute magnitude of 11.25.[5] According to the surveys carried out by the JapaneseAkari satellite and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Herschel measures between 14.768 and 17.385 kilometers in diameter and its surface has analbedo between 0.1870 and 0.256.[7][8][9][10][11]

See also

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References

[edit]
  1. ^abcde"2000 Herschel (1960 OA)".Minor Planet Center. Retrieved31 October 2018.
  2. ^"Herschel".Oxford English Dictionary (Online ed.). Oxford University Press. (Subscription orparticipating institution membership required.)
  3. ^abcSchmadel, Lutz D. (2007). "(2000) Herschel".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 162.doi:10.1007/978-3-540-29925-7_2001.ISBN 978-3-540-00238-3.
  4. ^abcdefgh"JPL Small-Body Database Browser: 2000 Herschel (1960 OA)" (2018-08-12 last obs.).Jet Propulsion Laboratory. Retrieved31 October 2018.
  5. ^abcdefg"LCDB Data for (2000) Herschel". Asteroid Lightcurve Database (LCDB). Retrieved13 March 2017.
  6. ^ab"Asteroid 2000 Herschel – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved26 October 2019.
  7. ^abcdMainzer, A. K.; Bauer, J. M.; Cutri, R. M.; Grav, T.; Kramer, E. A.; Masiero, J. R.; et al. (June 2016)."NEOWISE Diameters and Albedos V1.0".NASA Planetary Data System: EAR–A–COMPIL–5–NEOWISEDIAM–V1.0.Bibcode:2016PDSS..247.....M. Retrieved31 October 2018.
  8. ^abcMasiero, 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.S2CID 119293330.
  9. ^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.
  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. ^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. (catalog)
  12. ^abWarner, Brian D. (April 2011). "Upon Further Review: VI. An Examination of Previous Lightcurve Analysis from the Palmer Divide Observatory".The Minor Planet Bulletin.38 (2):96–101.Bibcode:2011MPBu...38...96W.ISSN 1052-8091.
  13. ^Nesvorný, 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.S2CID 119280014.
  14. ^Steel, D. I. (August 1985)."Collisions in the solar systems. II - Asteroid impacts upon Mars".Monthly Notices of the Royal Astronomical Society.215 (3):369–381.Bibcode:1985MNRAS.215..369S.doi:10.1093/mnras/215.3.369.ISSN 0035-8711.
  15. ^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.
  16. ^abElkins-Tanton, Linda T. (2010).Asteroids, Meteorites, and Comets. Infobase. p. 96.ISBN 9781438131863.

External links

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