Movatterモバイル変換


[0]ホーム

URL:


Jump to content
WikipediaThe Free Encyclopedia
Search

2054 Gawain

From Wikipedia, the free encyclopedia
Dark and elongated asteroid from the outer regions of the asteroid belt

2054 Gawain
Discovery[1]
Discovered byC. J. van Houten
I. van Houten-G.
T. Gehrels
Discovery sitePalomar Obs.
Discovery date24 September 1960
Designations
(2054) Gawain
Named after
Gawain(Arthurian legend)[2]
4097 P-L · 1973 FG1
main-belt · (outer)[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.52 yr (22,834 days)
Aphelion3.2591AU
Perihelion2.6716 AU
2.9653 AU
Eccentricity0.0991
5.11yr (1,865 days)
315.28°
0° 11m 34.8s / day
Inclination3.7886°
293.24°
183.97°
Physical characteristics
Dimensions17.28±4.94 km[4]
18.042±0.245 km[5][6]
19.95 km(derived)[3]
20.05±2.1 km[7]
20.77±0.63 km[8]
11.1098±0.0004h[9]
11.5±0.1 h[10]
11.581±0.0194 h[11]
0.0444(derived)[3]
0.06±0.04[4]
0.068±0.005[8]
0.0697±0.017[7]
0.073±0.008[5][6]
C[3]
12.00[5][8] · 12.5[1][3][4] · 12.507±0.010(R)[11] · 12.53±0.34(R)[10]

2054 Gawain, provisional designation4097 P-L, is a dark and elongatedasteroid from the outer regions of theasteroid belt, approximately 19 kilometers in diameter. Discovered during thePalomar–Leiden survey atPalomar Observatory in 1960, the asteroid was later named afterGawain, a knight of King Arthur'sRound Table in the Arthurian legend.[2]

Discovery

[edit]

Gawain was discovered on 24 September 1960, by Dutch astronomer coupleIngrid andCornelis van Houten, as well as Dutch–American astronomerTom Gehrels from images taken at thePalomar Observatory near San Diego, California, in the United States.[12]

Palomar–Leiden survey

[edit]

Thesurvey designation "P-L" stands forPalomar–Leiden, named after Palomar Observatory andLeiden Observatory, which collaborated on the fruitfulPalomar–Leiden survey in the 1960s. Gehrels used Palomar'sSamuel Oschin telescope (also known as the 48-inch Schmidt Telescope), and shipped thephotographic plates to Ingrid and Cornelis van Houten at Leiden Observatory whereastrometry was carried out. The trio are credited with the discovery ofseveral thousand asteroids.[13]

Orbit and classification

[edit]

Gawain orbits the Sun in theouter main-belt at a distance of 2.7–3.3 AU once every 5 years and 1 month (1,865 days). Its orbit has aneccentricity of 0.10 and aninclination of 4° with respect to theecliptic.[1]

The asteroid'sobservation arc begins 6 years prior to its official discovery observation, with aprecovery taken at the discovering Palomar Observatory in July 1954.[12]

Physical characteristics

[edit]

Gawain is an assumed carbonaceousC-type asteroid.[3]

Lightcurves

[edit]

In October 2001, a first rotationallightcurve ofGawain was obtained from photometric observations by an international collaboration of astronomers. Lightcurve analysis gave arotation period of 11.1098 hours with a high brightness variation of 0.69magnitude (U=2).[9] Additional lightcurves with a period of 11.581 and 11.5 hours and an amplitude of 0.65 and 1.05, respectively, were obtained by astronomers at thePalomar Transient Factory in California in 2011 and 2013 (U=2).[10][11] A high brightness amplitude typically indicates that the body has a non-spheroidal shape.

Diameter and albedo

[edit]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission,Gawain measures between 17.28 and 20.77 kilometers in diameter and its surface has analbedo between 0.06 and 0.073.[4][5][6][7][8] TheCollaborative Asteroid Lightcurve Link agrees with the results obtained by IRAS, and derives an albedo of 0.0444 and a diameter of 19.95 kilometers based on anabsolute magnitude of 12.5.[3]

Naming

[edit]

Thisminor planet was named after the figureGawain, King Arthur's nephew and a Knight of the Round Table in the Arthurian legend.[2] The approved naming citation was published by theMinor Planet Center on 13 October 1981 (M.P.C. 6421).[14]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 2054 Gawain (4097 P-L)" (2017-01-07 last obs.).Jet Propulsion Laboratory. Retrieved6 July 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(2054) Gawain".Dictionary of Minor Planet Names – (2054) Gawain.Springer Berlin Heidelberg. p. 166.doi:10.1007/978-3-540-29925-7_2055.ISBN 978-3-540-00238-3.
  3. ^abcdefg"LCDB Data for (2054) Gawain". Asteroid Lightcurve Database (LCDB). Retrieved6 July 2017.
  4. ^abcdNugent, C. R.; Mainzer, A.; Masiero, J.; Bauer, J.; Cutri, R. M.; Grav, T.; et al. (December 2015)."NEOWISE Reactivation Mission Year One: Preliminary Asteroid Diameters and Albedos".The Astrophysical Journal.814 (2): 13.arXiv:1509.02522.Bibcode:2015ApJ...814..117N.doi:10.1088/0004-637X/814/2/117. Retrieved6 July 2017.
  5. ^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.
  6. ^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. Retrieved6 July 2017.
  7. ^abcTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004)."IRAS Minor Planet Survey V6.0".NASA Planetary Data System.12: IRAS-A-FPA-3-RDR-IMPS-V6.0.Bibcode:2004PDSS...12.....T. Retrieved22 October 2019.
  8. ^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)
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2054) Gawain".Geneva Observatory. Retrieved6 July 2017.
  10. ^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. Retrieved6 July 2017.
  11. ^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. Retrieved6 July 2017.
  12. ^ab"2054 Gawain (4097 P-L)".Minor Planet Center. Retrieved6 July 2017.
  13. ^"Minor Planet Discoverers".Minor Planet Center. 11 June 2017. Retrieved6 July 2017.
  14. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved6 July 2017.


Minor planets
Asteroid
Distant minor planet
Comets
Other
Authority control databasesEdit this at Wikidata
Retrieved from "https://en.wikipedia.org/w/index.php?title=2054_Gawain&oldid=1292928523"
Categories:
Hidden categories:

[8]ページ先頭

©2009-2025 Movatter.jp