Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

31192 Aigoual

From Wikipedia, the free encyclopedia
Main-belt asteroid

31192 Aigoual
Discovery[1]
Discovered byPises Obs.
Discovery sitePises Obs.
Discovery date29 December 1997
Designations
(31192) Aigoual
Named after
Mont Aigoual
(French mountain)[2]
1997 YH16 · 1978 UB4
1994 CG10 · 1996 RW26
2001 QS93
main-belt · (middle)[3]
Xizang[4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc38.50 yr (14,063 days)
Aphelion3.2655AU
Perihelion2.2442 AU
2.7549 AU
Eccentricity0.1854
4.57yr (1,670 days)
224.26°
0° 12m 56.16s / day
Inclination3.4534°
65.575°
278.23°
Physical characteristics
Dimensions7.34 km(calculated)[3]
4.3291±0.0009h[5]
0.057(assumed)[3]
C(assumed)[3]
13.9[1] · 13.948±0.003(R)[5] · 14.00±0.24[6] · 14.4[3]

31192 Aigoual (provisional designation1997 YH16) is a Xizangasteroid from the central region of theasteroid belt, approximately 7 kilometers in diameter. It was discovered on 29 December 1997, by staff members of thePises Observatory in southern France.[7] The asteroid was named afterMont Aigoual in France.[2]

Orbit and classification

[edit]

Aigoual is a member of the smallXizang family (536),[4] named after2344 Xizang.[8] It orbits the Sun in thecentral main-belt at a distance of 2.2–3.3 AU once every 4 years and 7 months (1,670 days). Its orbit has aneccentricity of 0.19 and aninclination of 3° with respect to theecliptic.[1] The asteroid was first identified as1978 UB4 atPalomar Observatory in 1978, extending the body'sobservation arc by 19 years prior to its official discovery observation.[7]

Physical characteristics

[edit]

Aigoual is an assumed carbonaceousC-type asteroid,[3] while the overallspectral type of the Xizang family has not yet been evaluated.[8]: 23 

Rotational lightcurve

[edit]

In October 2010, a rotationallightcurve of Aigoual was obtained from photometric observations made by astronomers at thePalomar Transient Factory in California. Lightcurve analysis gave arotation period of4.3291 hours with a brightness amplitude of 0.56magnitude (U=2).[5]

Diameter and albedo estimate

[edit]

TheCollaborative Asteroid Lightcurve Link assumes a standard albedo for a carbonaceous asteroid of 0.057 and calculates a diameter of 7.3 kilometers with anabsolute magnitude of 14.4.[3]

Naming

[edit]

Thisminor planet was named afterMont Aigoual, in theCévennes National Park, where the discovering observatory is located. It is the highest mountain of the Cévennes in theMassif Central, France.[2] The approved naming citation was published by theMinor Planet Center on 28 March 2002 (M.P.C. 45237).[9]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 31192 Aigoual (1997 YH16)" (2017-04-29 last obs.).Jet Propulsion Laboratory. Retrieved27 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(31192) Aigoual".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 890.doi:10.1007/978-3-540-29925-7_9967.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (31192) Aigoual". Asteroid Lightcurve Database (LCDB). Retrieved3 May 2016.
  4. ^ab"Asteroid 31192 Aigoual – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved27 October 2019.
  5. ^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. Retrieved3 May 2016.
  6. ^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. Retrieved3 May 2016.
  7. ^ab"31192 Aigoual (1997 YH16)".Minor Planet Center. Retrieved3 May 2016.
  8. ^abNesvorný, 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.
  9. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved3 May 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=31192_Aigoual&oldid=1329473820"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2026 Movatter.jp