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2865 Laurel

From Wikipedia, the free encyclopedia
Main-belt asteroid

2865 Laurel
2865 Laurel orbit, and his position on 06 Jun 2011 (NASA Orbit Viewer applet)
Discovery[1]
Discovered byC. Jackson
Discovery siteJohannesburg Obs.
Discovery date31 July 1935
Designations
(2865) Laurel
Named after
Stan Laurel(film comedian)[2]
1935 OK · 1939 PA
1947 NF · 1951 ML
1972 QH
main-belt · (middle)[3]
Maria
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc81.62 yr (29,810 days)
Aphelion2.7406AU
Perihelion2.3812 AU
2.5609 AU
Eccentricity0.0702
4.10yr (1,497 days)
71.330°
0° 14m 25.8s / day
Inclination14.294°
321.79°
293.35°
Physical characteristics
Dimensions14.73±1.2 km(IRAS:3)[4]
14.79 km(derived)[3]
18.83±0.73 km[5]
24.99±0.37 km[6]
21.5±0.3h[7]
0.094±0.014[6]
0.142±0.013[5]
0.2242±0.043(IRAS:3)[4]
0.2438(derived)[3]
S[3][8]
11.20[6] · 11.24±0.30[8] · 11.3[1][3] · 11.40[4][5]

2865 Laurel, provisional designation1935 OK, is a stony Marianasteroid from the middle region of theasteroid belt, approximately 15 kilometers in diameter. It was discovered by English-born South African astronomerCyril Jackson atJohannesburg Observatory on 31 July 1935.[9] The asteroid was named after movie comedianStan Laurel.[2]

Orbit and classification

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Laurel orbits the Sun in thecentral main-belt at a distance of 2.4–2.7 AU once every 4 years and 1 month (1,497 days). Its orbit has aneccentricity of 0.07 and aninclination of 14° with respect to theecliptic.[1] Noprecoveries were taken and the asteroid'sobservation arc begins with its discovery observation in 1935.[9]

Physical characteristics

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Laurel has been characterized as a commonS-type asteroid byPanSTARRS' photometric survey.[8]

Rotation period

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A rotationallightcurve for this asteroid was obtained from photometric observations by French amateur astronomerPierre Antonini in September 2005. It gave a longer than averagerotation period of21.5±0.3 hours with a brightness variation of 0.15 inmagnitude (U=2).[7]

Diameter and albedo

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According to the space-based surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and NASA'sWide-field Infrared Survey Explorer with its subsequentNEOWISE mission, the asteroid measures between 14.7 and 25.0 kilometers in diameter and its surface has analbedo between 0.09 and 0.22.[4][5][6] TheCollaborative Asteroid Lightcurve Link agrees with IRAS and derives an albedo of 0.24 and a diameter 14.8 kilometers.[3]

Naming

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Thisminor planet was named after English-born slapstick film comedianStan Laurel (1890–1965). Together with Oliver Hardy (1892–1957), who was honored with the main-belt asteroid2866 Hardy, they formed the first great comedy duo inClassical Hollywood cinema.[2] The official naming citation was published by theMinor Planet Center on 1 September 1993 (M.P.C. 22496),[10] based on a suggestion byGareth V. Williams and others.[2]

References

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  1. ^abcd"JPL Small-Body Database Browser: 2865 Laurel (1935 OK)" (2017-03-12 last obs.).Jet Propulsion Laboratory. Retrieved14 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(2865) Laurel".Dictionary of Minor Planet Names – (2865) Laurel.Springer Berlin Heidelberg. p. 235.doi:10.1007/978-3-540-29925-7_2866.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (2865) Laurel". Asteroid Lightcurve Database (LCDB). Retrieved9 July 2016.
  4. ^abcdTedesco, 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.
  5. ^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)
  6. ^abcdMasiero, Joseph R.; Mainzer, A. K.; Grav, T.; Bauer, J. M.; Cutri, R. M.; Nugent, C.; et al. (November 2012)."Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids".The Astrophysical Journal Letters.759 (1): 5.arXiv:1209.5794.Bibcode:2012ApJ...759L...8M.doi:10.1088/2041-8205/759/1/L8. Retrieved9 July 2016.
  7. ^abBehrend, Raoul."Asteroids and comets rotation curves – (2865) Laurel".Geneva Observatory. Retrieved9 July 2016.
  8. ^abcVeres, 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. Retrieved9 July 2016.
  9. ^ab"2865 Laurel (1935 OK)".Minor Planet Center. Retrieved9 July 2016.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved9 July 2016.

External links

[edit]
Minor planets
Asteroid
Distant minor planet
Comets
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Authority control databasesEdit this at Wikidata
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