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1633 Chimay

From Wikipedia, the free encyclopedia
Themistian asteroid

1633 Chimay
Lightcurve based 3D-model ofChimay
Discovery[1]
Discovered byS. Arend
Discovery siteUccle Obs.
Discovery date3 March 1929
Designations
(1633) Chimay
Named after
Chimay(Belgian town)[2]
1929 EC · 1941 KF
1946 HC · 1948 RO
1951 AM · 1952 HY3
1954 SS · 1955 XN
1972 VM1 · A917 BB
main-belt · Themis[3]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc100.02 yr (36,531 days)
Aphelion3.5907AU
Perihelion2.7980 AU
3.1943 AU
Eccentricity0.1241
5.71yr (2,085 days)
237.33°
0° 10m 21.36s / day
Inclination2.6759°
114.08°
65.539°
Physical characteristics
Dimensions36.07 km(derived)[3]
36.12±3.1 km(IRAS:3)[4]
36.26±0.86 km[5]
37.428±0.466[6]
37.732±0.426 km[7]
6.58±0.01 h[8]
6.59064±0.00005 h[9]
6.5911±0.0001h[10]
6.6367±0.0038 h[11]
0.0781(derived)[3]
0.0785±0.0135[7]
0.080±0.014[6]
0.0854±0.017(IRAS:3)[4]
0.088±0.005[5]
S[3]
10.36±0.17(R)[8] · 10.481±0.002(R)[11] · 10.5[5][7] · 10.6[1][3] · 10.97±0.06[12]

1633 Chimay, provisional designation1929 EC, is a Themistianasteroid from the outer region of theasteroid belt, approximately 37 kilometers in diameter.

It was discovered on 3 March 1929, by Belgian astronomerSylvain Arend at theRoyal Observatory of Belgium in Uccle.[13] Five nights later, the body was independently discovered byMax Wolf atHeidelberg Observatory in southern Germany.[2] It was later named for the Belgian town ofChimay.[2]

Classification and orbit

[edit]

Chimay is a member of theThemis family, a dynamical family of asteroids with nearly coplanarecliptical orbits. It orbits the Sun in theouter main-belt at a distance of 2.8–3.6 AU once every 5 years and 9 months (2,085 days). Its orbit has aneccentricity of 0.12 and aninclination of 3° with respect to the ecliptic.[1]Chimay was first identified asA917 BB at Heidelberg in 1917, extending the body'sobservation arc by 12 years prior to its official discovery observation.[13]

Physical characteristics

[edit]

Several rotationallightcurves were obtained from photometric observations. Lightcurve analysis gave a well-defined, concurringrotation period of 6.58–6.63 hours with a brightness variation between 0.31 and 0.58magnitude (U=3/3-/2).[8][9][10][11][14]

According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Chimay measures between 36.1 and 37.7 kilometers in diameter, and its surface has a lowalbedo between 0.079 and 0.089.[4][5][6][7] In accordance with the space-based surveys, theCollaborative Asteroid Lightcurve Link (CALL) derives an albedo of 0.078, and calculates a diameter of 36.1 kilometers. CALL also classifiesChimay as aS-type rather than a carbonaceousC-type asteroid.[3]

Naming

[edit]

Thisminor planet was named after the Belgian townChimay, home of the discoverer, who also co-discoveredComet Arend–Roland.[2] The officialnaming citation was published by theMinor Planet Center on 20 February 1976 (M.P.C. 3931).[15]

References

[edit]
  1. ^abcd"JPL Small-Body Database Browser: 1633 Chimay (1929 EC)" (2017-01-28 last obs.).Jet Propulsion Laboratory. Retrieved30 June 2017.
  2. ^abcdSchmadel, Lutz D. (2007). "(1633) Chimay".Dictionary of Minor Planet Names – (1633) Chimay.Springer Berlin Heidelberg. p. 130.doi:10.1007/978-3-540-29925-7_1634.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1633) Chimay". Asteroid Lightcurve Database (LCDB). Retrieved1 May 2016.
  4. ^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.
  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. ^abcMasiero, Joseph R.; Grav, T.; Mainzer, A. K.; Nugent, C. R.; Bauer, J. M.; Stevenson, R.; et al. (August 2014)."Main-belt Asteroids with WISE/NEOWISE: Near-infrared Albedos".The Astrophysical Journal.791 (2): 11.arXiv:1406.6645.Bibcode:2014ApJ...791..121M.doi:10.1088/0004-637X/791/2/121. Retrieved8 December 2016.
  7. ^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. Retrieved1 May 2016.
  8. ^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. Retrieved7 January 2016.
  9. ^abHanus, J.; Broz, M.; Durech, J.; Warner, B. D.; Brinsfield, J.; Durkee, R.; et al. (November 2013)."An anisotropic distribution of spin vectors in asteroid families".Astronomy and Astrophysics.559: 19.arXiv:1309.4296.Bibcode:2013A&A...559A.134H.doi:10.1051/0004-6361/201321993. Retrieved7 January 2016.
  10. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1633) Chimay".Geneva Observatory. Retrieved1 May 2016.
  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. Retrieved1 May 2016.
  12. ^Veres, 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. Retrieved1 May 2016.
  13. ^ab"1633 Chimay (1929 EC)".Minor Planet Center. Retrieved1 May 2016.
  14. ^Brinsfield, James W. (October 2008)."Asteroid Lightcurve Analysis at the Via Capote Observatory: 2nd Quarter 2008".The Minor Planet Bulletin.35 (4):179–181.Bibcode:2008MPBu...35..179B.ISSN 1052-8091. Retrieved7 January 2016.
  15. ^Schmadel, Lutz D. "Appendix – Publication Dates of the MPCs".Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008). Springer Berlin Heidelberg. p. 221.doi:10.1007/978-3-642-01965-4.ISBN 978-3-642-01964-7.

External links

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