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1764 Cogshall

From Wikipedia, the free encyclopedia
Carbonaceous Themistian asteroid

1764 Cogshall
Discovery[1]
Discovered byIndiana University
(Indiana Asteroid Program)
Discovery siteGoethe Link Obs.
Discovery date7 November 1953
Designations
(1764) Cogshall
Named after
Wilbur A. Cogshall[2]
(professor of astronomy at IU)
1953 VM1 · 1935 MF
1939 CC · 1942 VB
1951 LC · 1952 SM
1953 XJ · 1964 XG
1967 GO · 1969 TN2
main-belt · (outer)
Themis[3][4][5]
Orbital characteristics[1]
Epoch 4 September 2017 (JD 2458000.5)
Uncertainty parameter 0
Observation arc82.02 yr (29,956 days)
Aphelion3.4671AU
Perihelion2.7193 AU
3.0932 AU
Eccentricity0.1209
5.44yr (1,987 days)
84.951°
0° 10m 52.32s / day
Inclination2.2355°
152.23°
79.719°
Physical characteristics
Dimensions25.14±0.64 km[6]
26.13 km(derived)[3]
26.21±2.0 km[7]
26.970±0.232 km[8]
29.671±0.179 km[9]
3.624±0.0052h(R)[10]
3.62417±0.00007 h[11]
3.630±0.0052 h(S)[10]
0.0606±0.0086[9]
0.0712(derived)[3]
0.0852±0.015[7]
0.094±0.005[6]
0.109±0.010[8]
S/C(generically assumed)[3]
11.20[6][7] · 11.248±0.002(R)[10] · 11.3[9] · 11.4[1][3]

1764 Cogshall, provisional designation1953 VM1, is a carbonaceous Themistianasteroid from the outer regions of theasteroid belt, approximately 26 kilometers in diameter. It was discovered on 7 November 1953 by astronomers of theIndiana Asteroid Program atGoethe Link Observatory in Indiana, United States.[12] The asteroid was named afterWilbur Cogshall, professor of astronomy atIndiana University.[2]

Orbit and classification

[edit]

Cogshall is a Themistian asteroid that belongs to theThemis family (602),[4][5] a very largefamily of carbonaceous asteroids named after24 Themis.[13]: 23  It orbits the Sun in theouter main belt at a distance of 2.7–3.5 AU once every 5 years and 5 months (1,987 days). Its orbit has aneccentricity of 0.12 and aninclination of 2° concerning to theecliptic.[1]

The asteroid was first identified as1935 MF atJohannesburg Observatory in June 1935. The body'sobservation arc begins with its identification as1939 CC atTurku Observatory in February 1939, more than 14 years before its official discovery observation at Goethe Link.[12]

Physical characteristics

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Rotation period

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In May 2005, French amateur astronomerPierre Antonini obtained a rotationallightcurve ofCogshall from photometric observations. Lightcurve analysis gave a well-definedrotation period of 3.62417 hours with a brightness variation of 0.21magnitude (U=3).[11]

Observations at thePalomar Transient Factory in 2012 gave a concurring period of 3.624 and 3.630 hours with an amplitude of 0.22 and 0.20 magnitude in the R- and S-band, respectively (U=2/2).[10]

Diameter and albedo

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According to the surveys carried out by the Infrared Astronomical SatelliteIRAS, the JapaneseAkari satellite, and theNEOWISE mission of NASA'sWide-field Infrared Survey Explorer,Cogshall measures between 25.14 and 29.671 kilometers in diameter, and its surface has analbedo between 0.0606 and 0.109.[6][7][8][9]

TheCollaborative Asteroid Lightcurve Link derives an albedo of 0.0712 and a diameter of 26.13 kilometers based on anabsolute magnitude of 11.4.[3]

Naming

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Thisminor planet was named after American astronomerWilbur A. Cogshall, a professor of astronomy atIndiana University and director of theKirkwood Observatory for more than four decades (1900–1944). His research included visualbinary stars and the photography ofsolar eclipses. The name was proposed byFrank K. Edmondson, who initiated theIndiana Asteroid Program.[2][14] TheMinor Planet Center published the officialnaming citation on 20 February 1971 (M.P.C. 3143).[15]

References

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  1. ^abcd"JPL Small-Body Database Browser: 1764 Cogshall (1953 VM1)" (2017-07-05 last obs.).Jet Propulsion Laboratory. Retrieved6 September 2017.
  2. ^abcSchmadel, Lutz D. (2007). "(1764) Cogshall".Dictionary of Minor Planet Names.Springer Berlin Heidelberg. p. 141.doi:10.1007/978-3-540-29925-7_1765.ISBN 978-3-540-00238-3.
  3. ^abcdef"LCDB Data for (1764) Cogshall". Asteroid Lightcurve Database (LCDB). Retrieved6 September 2017.
  4. ^ab"Asteroid 1764 Cogshall – Nesvorny HCM Asteroid Families V3.0".Small Bodies Data Ferret. Retrieved31 October 2019.
  5. ^ab"Asteroid 1764 Cogshall – Proper Elements". AstDyS-2, Asteroids – Dynamic Site. Retrieved31 October 2019.
  6. ^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)
  7. ^abcdTedesco, E. F.; Noah, P. V.; Noah, M.; Price, S. D. (October 2004). "IRAS Minor Planet Survey V6.0".NASA Planetary Data System.Bibcode:2004PDSS...12.....T.
  8. ^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.
  9. ^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.
  10. ^abcdWaszczak, 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.
  11. ^abBehrend, Raoul."Asteroids and comets rotation curves – (1764) Cogshall".Geneva Observatory. Retrieved6 September 2017.
  12. ^ab"1764 Cogshall (1953 VM1)".Minor Planet Center. Retrieved6 September 2017.
  13. ^Nesvorný, D.; Broz, M.; Carruba, V. (December 2014). "Identification and Dynamical Properties of Asteroid Families".Asteroids IV. pp. 297–321.arXiv:1502.01628.Bibcode:2015aste.book..297N.doi:10.2458/azu_uapress_9780816532131-ch016.ISBN 9780816532131.
  14. ^Lauren J. Bryant."Farseeing and Abiding at IU". Indiana University. Retrieved6 September 2017.
  15. ^Schmadel, Lutz D. (2009). "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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