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6042 Cheshirecat

From Wikipedia, the free encyclopedia
Mars-crossing asteroid

6042 Cheshirecat
Discovery[1]
Discovered byA. Natori
T. Urata
Discovery siteJCPM Yakiimo Stn.
Discovery date23 November 1990
Designations
(6042) Cheshirecat
Pronunciation/ˈɛʃərkæt/  · /ˈɛʃɪərkæt/
Named after
Cheshire Cat
(Alice in Wonderland)[2]
1990 WW2
Mars-crosser[1][3][4]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc36.84 yr (13,454 days)
Aphelion4.4295AU
Perihelion1.6505 AU
3.0400 AU
Eccentricity0.4571
5.30yr (1,936 days)
34.629°
0° 11m 9.24s / day
Inclination15.885°
88.606°
286.27°
Physical characteristics
Dimensions14.12±0.20 km[5]
14.64 km(calculated)[4]
10.049±0.004h[6]
10.050±0.002 h[7]
0.109±0.004[5]
0.057(assumed)[4]
XL[8] · K[9] · C[4]
12.00[9] · 12.30[5] · 12.77±0.62[8] · 12.9[1][4]

6042 Cheshirecat (/ˈɛʃərkæt/or/ˈɛʃɪərkæt/), provisional designation1990 WW2, is an eccentric, rare-typeasteroid and largeMars-crosser from the outer regions of theasteroid belt, approximately 14 kilometers in diameter. It was discovered by Japanese astronomersAkira Natori andTakeshi Urata at theJCPM Yakiimo Station on 23 November 1990.[3] It was named for theCheshire Cat from the novelAlice's Adventures in Wonderland.[2]

Classification and orbit

[edit]

Cheshirecat is aMars-crossing asteroid, as it crosses the orbit ofMars at 1.666 AU. It orbits the Sun at a distance of 1.65–4.43 AU once every 5 years and 4 months (1,936 days). Its orbit has aneccentricity of 0.46 and aninclination of 16° with respect to theecliptic.[1]

The body'sobservation arc begins 11 years prior to its official discovery observation, with aprecovery taken at theSiding Spring Observatory in August 1979.[3]

Physical characteristics

[edit]

According to photometry from theSloan Digital Sky Survey,Cheshirecat is a rareK-type asteroid.[9] The asteroid has also been characterized as a XL-type – which transitions from theX-type to theL-type asteroid – byPan-STARRS photometric survey.[8]

Lightcurves

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In December 2006, a rotationallightcurve ofCheshirecat was obtained from photometric observations by American astronomerRobert Stephens. Lightcurve analysis gave arotation period of 10.050 hours with a brightness variation of 0.40magnitude (U=3-).[7] In September 2011, another lightcurve, obtained at the Oakley Southern Sky Observatory (E09), Australia, gave a concurring period of 10.050 hours and an amplitude of 0.20 (U=3-)[6]

Diameter and albedo

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According to the survey carried out by the JapaneseAkari satellite,Cheshirecat measures 14.12 kilometers in diameter and its surface has analbedo of 0.109.[5] TheCollaborative Asteroid Lightcurve Link assumes a standard albedo forcarbonaceous asteroids of 0.057 and calculates a diameter of 14.64 kilometers based on anabsolute magnitude of 12.9.[4]

Naming

[edit]

Thisminor planet was named for theCheshire Cat, a cat appearing inLewis Carroll's famous fairy taleAlice in Wonderland. The cat is known for its distinctive mischievous grins and eyes that linger after it has already faded away. The asteroid's name and citation was proposed by co-discovererTakeshi Urata.[2] The approved naming citation was published by theMinor Planet Center on 2 February 1999 (M.P.C. 33786).[10]

References

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  1. ^abcde"JPL Small-Body Database Browser: 6042 Cheshirecat (1990 WW2)" (2016-06-14 last obs.).Jet Propulsion Laboratory. Retrieved29 June 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(6042) Cheshirecat".Dictionary of Minor Planet Names – (6042) Cheshirecat.Springer Berlin Heidelberg. p. 505.doi:10.1007/978-3-540-29925-7_5607.ISBN 978-3-540-00238-3.
  3. ^abc"6042 Cheshirecat (1990 WW2)".Minor Planet Center. Retrieved29 June 2017.
  4. ^abcdef"LCDB Data for (6042) Cheshirecat". Asteroid Lightcurve Database (LCDB). Retrieved29 June 2017.
  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. ^abFolberth, James; Casimir, Serick; Dou, Yueheng; Evans, Davis; Foulkes, Thomas; Haenftling, Miranda; et al. (April 2012)."Asteroid Lightcurve Analysis at the Oakley Southern Sky Observatory: 2011 July-September".The Minor Planet Bulletin.39 (2):51–55.Bibcode:2012MPBu...39...51F.ISSN 1052-8091. Retrieved29 June 2017.
  7. ^abStephens, Robert D. (April 2012)."Asteroids Observed from GMARS and Santana Observatories: 2011 October- December".The Minor Planet Bulletin.39 (2):80–82.Bibcode:2012MPBu...39...80S.ISSN 1052-8091. Retrieved29 June 2017.
  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. Retrieved29 June 2017.
  9. ^abcCarry, B.; Solano, E.; Eggl, S.; DeMeo, F. E. (April 2016)."Spectral properties of near-Earth and Mars-crossing asteroids using Sloan photometry".Icarus.268:340–354.arXiv:1601.02087.Bibcode:2016Icar..268..340C.doi:10.1016/j.icarus.2015.12.047. Retrieved29 June 2017.
  10. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved29 June 2017.

External links

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