Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

3640 Gostin

From Wikipedia, the free encyclopedia
Main-belt asteroid

3640 Gostin
Discovery[1]
Discovered byC. Shoemaker
E. Shoemaker
Discovery sitePalomar Obs.
Discovery date11 October 1985
Designations
(3640) Gostin
Named after
Victor Gostin[1]
(Australian geologist)
1985 TR3 · 1955 SS
1960 CB · 1970 CS
1972 VJ1
main-belt[1][2] · (inner)
Flora[3][4]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc61.63yr (22,511 d)
Aphelion2.4175AU
Perihelion2.0311 AU
2.2243 AU
Eccentricity0.0869
3.32 yr (1,212 d)
224.62°
0° 17m 49.56s / day
Inclination4.3118°
289.19°
155.59°
Physical characteristics
7.148±0.088 km[5]
7.613±0.096 km[6]
8.58 km(calculated)[3]
3.26±0.05 h[7]
3.263±0.0009 h[8]
3.263±0.003 h[9]
3.2641±0.0005 h[10]
0.2127±0.0446[6]
0.239±0.036[5]
0.24(assumed)[3]
SMASS =S[2][3]
12.26±0.14(R)[7]
12.398±0.001(R)[8]
12.5[2][3]
12.62±0.20[11]
12.9[6]

3640 Gostin, provisional designation1985 TR3, is a stony Florianasteroid from the inner regions of theasteroid belt, approximately 8 kilometers (5 miles) in diameter. It was discovered on 11 October 1985, by American astronomer coupleCarolyn andEugene Shoemaker at thePalomar Observatory in California.[1] TheS-type asteroid has arotation period of 3.26 hours.[3] It was named for Australian geologistVictor Gostin.[1]

Orbit and classification

[edit]

Gostin is a member of theGondolatsch-cluster within theFlora family (402),[3][4] a giantasteroid family and the largest family of stony asteroids in the main-belt,[12]

It orbits the Sun in theinner main-belt at a distance of 2.0–2.4 AU once every 3 years and 4 months (1,212 days;semi-major axis of 2.22 AU). Its orbit has aneccentricity of 0.09 and aninclination of 4° with respect to theecliptic.[2] The body'sobservation arc begins with its first observation as1955 SS at theGoethe Link Observatory in September 1955, or 30 years prior to its official discovery observation at Palomar.[1]

Physical characteristics

[edit]

In theSMASS classification,Gostin is a common, stonyS-type asteroid.[2]

Rotation period

[edit]

In March 2010, a rotationallightcurve ofGostin was obtained fromphotometric observations at theOakley Southern Sky Observatory. Lightcurve analysis gave a well-definedrotation period of 3.2641 hours with a brightness variation of 0.40magnitude (U=3).[10] Concurring lightcurves were also obtained at thePalomar Transient Factory and at the Etscorn Campus Observatory (U=3/2/3).[3][7][8][9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Gostin measures 7.148 and 7.613 kilometers in diameter and its surface has analbedo of 0.239 and 0.2127, respectively.[5][6] TheCollaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from8 Flora, theparent body of the Flora family – and calculates a diameter of 8.58 kilometers based on anabsolute magnitude of 12.5.[3]

Naming

[edit]

Thisminor planet was named by the discoverers after Australian geologistVictor Gostin (born 1940) of theUniversity of Adelaide, who in the 1980s discovered the ejecta layer from theAcraman bolide impact at a distance of 300 kilometers from the impact site, withinEdiacaran sedimentary rocks of theFlinders Ranges,South Australia, which enabled the impact to be dated at ~580 Ma.[1][13] The official naming citation was published by theMinor Planet Center on 2 February 1988 (M.P.C. 12808).[14]

References

[edit]
  1. ^abcdefg"3640 Gostin (1985 TR3)".Minor Planet Center. Retrieved15 May 2018.
  2. ^abcdef"JPL Small-Body Database Browser: 3640 Gostin (1985 TR3)" (2017-05-05 last obs.).Jet Propulsion Laboratory. Retrieved15 May 2018.
  3. ^abcdefghi"LCDB Data for (3640) Gostin". Asteroid Lightcurve Database (LCDB). Retrieved15 May 2018.
  4. ^ab"Asteroid 3669 Vertinskij".Small Bodies Data Ferret. Retrieved15 May 2018.
  5. ^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.
  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.S2CID 35447010. (catalog)
  7. ^abcChang, Chan-Kao;Ip, Wing-Huen; Lin, Hsing-Wen; Cheng, Yu-Chi; Ngeow, Chow-Choong; Yang, Ting-Chang; et al. (June 2014). "313 New Asteroid Rotation Periods from Palomar Transient Factory Observations".The Astrophysical Journal.788 (1): 21.arXiv:1405.1144.Bibcode:2014ApJ...788...17C.doi:10.1088/0004-637X/788/1/17.S2CID 51100134.
  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.S2CID 8342929.
  9. ^abKlinglesmith, Daniel A. III; Hendrickx, Sebastian; Madden, Karl; Montgomery, Samuel (April 2016). "Lightcurves for Shape/Spin Models".The Minor Planet Bulletin.43 (2):123–128.Bibcode:2016MPBu...43..123K.ISSN 1052-8091.
  10. ^abAlbers, Kenda; Kragh, Katherine; Monnier, Adam; Pligge, Zachary; Stolze, Kellen; West, Josh; et al. (October 2010). "Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2009 October thru 2010 April".The Minor Planet Bulletin.37 (4):152–158.Bibcode:2010MPBu...37..152A.ISSN 1052-8091.
  11. ^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.S2CID 53493339.
  12. ^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.
  13. ^Gostin, V. A.; Haines, P. W.; Jenkins, R. J. F.; Compston, W.; Williams, I. S. (July 1986). "Impact ejecta horizon within late Precambrian shales, Adelaide Geosyncline, South Australia".Science.233 (4760):198–200.Bibcode:1986Sci...233..198G.doi:10.1126/science.233.4760.198.ISSN 0036-8075.PMID 17737290.S2CID 11307364.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved15 May 2018.

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=3640_Gostin&oldid=1313183162"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp