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5635 Cole

From Wikipedia, the free encyclopedia
Main-belt asteroid

5635 Cole
Shape model ofCole from itslightcurve
Discovery[1]
Discovered byS. J. Bus
Discovery siteSiding Spring Obs.
Discovery date2 March 1981
Designations
(5635) Cole
Named after
Joshua Cole[1]
(fictional character)
1981 ER5 · 1986 XC5
1988 CO5
main-belt[1][2] · (inner)
background[3]
Orbital characteristics[2]
Epoch 23 March 2018 (JD 2458200.5)
Uncertainty parameter 0
Observation arc37.20yr (13,588 d)
Aphelion3.0272AU
Perihelion1.7431 AU
2.3851 AU
Eccentricity0.2692
3.68 yr (1,345 d)
248.82°
0° 16m 3.36s / day
Inclination7.3102°
274.08°
54.118°
Physical characteristics
3.51±0.80 km[4]
4.263±0.620 km[5][6]
4.71 km(calculated)[7]
5.792±0.001 h[8]
5.7937±0.0001 h[9]
0.20(assumed)[7]
0.29±0.14[4]
0.294±0.100[5][6]
S(assumed)[7]
LS(SDSS-MOC)[10]
13.8[6]
14.0[2][7]
14.33[4]

5635 Cole (prov. designation:1981 ER5) is abackground asteroid from the inner regions of theasteroid belt, approximately 4 kilometers (2.5 miles) in diameter. It was discovered on 2 March 1981, by American astronomerSchelte Bus at theSiding Spring Observatory in Australia.[1] TheL/S-type asteroid has arotation period of 5.79 hours.[7] It was named after the fictional characterJoshua Cole.[1]

Orbit and classification

[edit]

Cole is a non-family asteroid of the main belt'sbackground population when applying thehierarchical clustering method to itsproper orbital elements.[3] It orbits the Sun in theinner main-belt at a distance of 1.7–3.0 AU once every 3 years and 8 months (1,345 days;semi-major axis of 2.39 AU). Its orbit has aneccentricity of 0.27 and aninclination of 7° with respect to theecliptic.[2] The body'sobservation arc begins with aprecovery taken at the discovering Siding Spring Observatory on 9 February 1981, or four weeks prior to its official discovery observation.[1]

Naming

[edit]

Thisminor planet was named after fictional characterJoshua Cole in the novelCole of Spyglass Mountain (1923) byArthur Preston Hankins. The protagonist, reminiscent of Oliver Twist, is an amateur astronomer in a dystopian society where boys receive numbers instead of names. In the novel, Cole's number isList of minor planets: 5001–6000#635 and corresponds to this asteroid's numbering.[1] The official naming citation was prepared byDavid H. Levy and published by theMinor Planet Center on 14 December 1997 (M.P.C. 31024).[11]

Physical characteristics

[edit]

In the Moving Object Catalog of theSloan Digital Sky Survey,Cole has aspectral type is closest to anL-type asteroid followed by the common, stonyS-type.[10] TheCollaborative Asteroid Lightcurve Link also assume it to be an S-type asteroid.[7]

Rotation period

[edit]

In September 2004, two rotationallightcurves ofCole were obtained fromphotometric observations byDonald Pray,Silvano Casulli,René Roy. Lightcurve analysis gave a well-definedrotation period of 5.792 and 5.7937 hours with a brightness amplitude of 0.33 and 0.30magnitude, respectively (U=3/3).[8][9]

Diameter and albedo

[edit]

According to the survey carried out by theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Cole measures between 3.51 and 4.263 kilometers in diameter and its surface has analbedo between 0.29 and 0.294,[4][5][6] while theCollaborative Asteroid Lightcurve Link assumes a standard albedo for a stony asteroids of 0.20, and calculates a diameter of 4.71 kilometers based on anabsolute magnitude of 14.0.[7]

References

[edit]
  1. ^abcdefg"5635 Cole (1981 ER5)".Minor Planet Center. Retrieved16 May 2018.
  2. ^abcd"JPL Small-Body Database Browser: 5635 Cole (1981 ER5)" (2018-04-24 last obs.).Jet Propulsion Laboratory. Retrieved16 May 2018.
  3. ^ab"Asteroid 5635 Cole".Small Bodies Data Ferret. Retrieved15 May 2018.
  4. ^abcdNugent, C. R.; Mainzer, A.; Bauer, J.; Cutri, R. M.; Kramer, E. A.; Grav, T.; et al. (September 2016)."NEOWISE Reactivation Mission Year Two: Asteroid Diameters and Albedos".The Astronomical Journal.152 (3): 12.arXiv:1606.08923.Bibcode:2016AJ....152...63N.doi:10.3847/0004-6256/152/3/63.
  5. ^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.S2CID 118745497.
  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. ^abcdefg"LCDB Data for (5635) Cole". Asteroid Lightcurve Database (LCDB). Retrieved16 May 2018.
  8. ^abPray, Donald P. (September 2005)."Lightcurve analysis of asteroids 106, 752, 847, 1057, 1630, 1670, 1927 1936, 2426, 2612, 2647, 4087, 5635, 5692, and 6235"(PDF).Minor Planet Bulletin.32 (3):48–51.Bibcode:2005MPBu...32...48P.ISSN 1052-8091. Archived fromthe original(PDF) on 18 March 2020. Retrieved22 March 2020.
  9. ^abBehrend, Raoul."Asteroids and comets rotation curves – (5635) Cole". Geneva Observatory. Retrieved16 May 2018.
  10. ^abCarvano, J. M.; Hasselmann, P. H.; Lazzaro, D.; Mothé-Diniz, T. (February 2010)."SDSS-based taxonomic classification and orbital distribution of main belt asteroids".Astronomy and Astrophysics.510: 12.Bibcode:2010A&A...510A..43C.doi:10.1051/0004-6361/200913322. Retrieved30 October 2019.(PDS data set)
  11. ^"MPC/MPO/MPS Archive".Minor Planet Center. Retrieved16 May 2018.

External links

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