Astronomy:2054 Gawain

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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 afterGawain (Arthurian legend)[2]
4097 P-L · 1973 FG1
Minor planet categorymain-belt · (outer) [3]
Orbital characteristics [1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc62.52 yr (22,834 days)
|{{{apsis}}}|helion}}3.2591 AU
|{{{apsis}}}|helion}}2.6716 AU
2.9653 AU
Eccentricity0.0991
Orbital period5.11 yr (1,865 days)
Mean anomaly315.28°
Mean motion0° 11m 34.8s / day
Inclination3.7886°
Longitude of ascending node293.24°
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]
Rotation period11.1098±0.0004 h[9]
11.5±0.1 h[10]
11.581±0.0194 h[11]
Geometric albedo0.0444 (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]
Absolute magnitude (H)12.00[5][8] · 12.5[1][3][4] · 12.507±0.010 (R)[11] · 12.53±0.34 (R)[10]


2054 Gawain, provisional designation 4097 P-L, is a dark and elongated asteroid from the outer regions of the asteroid belt, approximately 19 kilometers in diameter. Discovered during the Palomar–Leiden survey at Palomar Observatory in 1960, the asteroid was later named after Gawain, a knight of King Arthur's Round Table in the Arthurian legend.[2]

Discovery

Gawain was discovered on 24 September 1960, by Dutch astronomer couple Ingrid and Cornelis van Houten, as well as Dutch–American astronomer Tom Gehrels from images taken at the Palomar Observatory near San Diego, California, in the United States.[12]

Palomar–Leiden survey

Orbit and classification

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

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

Physical characteristics

Gawain is an assumed carbonaceous C-type asteroid.[3]

Lightcurves

In October 2001, a first rotational lightcurve of Gawain was obtained from photometric observations by an international collaboration of astronomers. Lightcurve analysis gave a rotation period of 11.1098 hours with a high brightness variation of 0.69 magnitude ({{{1}}}).[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 the Palomar Transient Factory in California in 2011 and 2013 ({{{1}}}).[10][11] A high brightness amplitude typically indicates that the body has a non-spheroidal shape.

Diameter and albedo

According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite, and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Gawain measures between 17.28 and 20.77 kilometers in diameter and its surface has an albedo between 0.06 and 0.073.[4][5][6][7][8] The Collaborative 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 an absolute magnitude of 12.5.[3]

Naming

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

References

  1. ↑ 1.0 1.1 1.2 1.3 "JPL Small-Body Database Browser: 2054 Gawain (4097 P-L)". Jet Propulsion Laboratory. https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2002054. 
  2. ↑ 2.0 2.1 2.2 Schmadel, 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. ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 "LCDB Data for (2054) Gawain". Asteroid Lightcurve Database (LCDB). http://www.minorplanet.info/PHP/generateOneAsteroidInfo.php?AstInfo=2054%7CGawain. 
  4. ↑ 4.0 4.1 4.2 4.3 Nugent, 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. doi:10.1088/0004-637X/814/2/117. Bibcode: 2015ApJ...814..117N. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015ApJ...814..117N. Retrieved 6 July 2017. 
  5. ↑ 5.0 5.1 5.2 5.3 Mainzer, 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. doi:10.1088/0004-637X/741/2/90. Bibcode: 2011ApJ...741...90M. 
  6. ↑ 6.0 6.1 6.2 Masiero, 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. doi:10.1088/0004-637X/741/2/68. Bibcode: 2011ApJ...741...68M. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2011ApJ...741...68M. Retrieved 6 July 2017. 
  7. ↑ 7.0 7.1 7.2 Tedesco, 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. https://sbnarchive.psi.edu/pds3/iras/IRAS_A_FPA_3_RDR_IMPS_V6_0/data/diamalb.tab. Retrieved 22 October 2019. 
  8. ↑ 8.0 8.1 8.2 8.3 Usui, 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. doi:10.1093/pasj/63.5.1117. Bibcode: 2011PASJ...63.1117U.  (online, AcuA catalog p. 153)
  9. ↑ 9.0 9.1 Behrend, Raoul. "Asteroids and comets rotation curves – (2054) Gawain". Geneva Observatory. http://obswww.unige.ch/~behrend/page4cou.html#002054. 
  10. ↑ 10.0 10.1 10.2 Chang, Chan-Kao (June 2014). "313 New Asteroid Rotation Periods from Palomar Transient Factory Observations". The Astrophysical Journal 788 (1): 21. doi:10.1088/0004-637X/788/1/17. Bibcode: 2014ApJ...788...17C. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2014ApJ...788...17C. Retrieved 6 July 2017. 
  11. ↑ 11.0 11.1 11.2 Waszczak, 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. doi:10.1088/0004-6256/150/3/75. Bibcode: 2015AJ....150...75W. http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2015AJ....150...75W. Retrieved 6 July 2017. 
  12. ↑ 12.0 12.1 "2054 Gawain (4097 P-L)". Minor Planet Center. https://www.minorplanetcenter.net/db_search/show_object?object_id=2054. 
  13. ↑ "MPC/MPO/MPS Archive". Minor Planet Center. https://www.minorplanetcenter.net/iau/ECS/MPCArchive/MPCArchive_TBL.html. 
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