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1836 Komarov
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Carbonaceous main-belt asteroid
October 2019
yes
1836 Komarov
#D6D6D6
001836-asteroid shape model (1836) Komarov.png
Shape model of Komarov from its lightcurve
26 July 1971
N. Chernykh
Crimean Astrophysical Obs.
(1836) Komarov
1971 OT1952 KA 11952 MT1961 JG1962 SG
Vladimir Komarov (Soviet cosmonaut)
main-belt(middle)Dora
16 February 2017 (JD 2457800.5)
0
63.89 yr (23,334 days)
3.3187 AU
2.2523 AU
2.7855 AU
0.1914
4.65 yr (1,698 days)
308.73°
0.2120 ms / day
7.0195°
272.76°
12.344°
21.16 km (calculated)21.55 6.10 km21.84 6.55 km22.240 0.304 km22.86 0.73 km25.40 9.32 km
8.8015 0.0004 h9.695 0.005 hLCDB-Caspari-2008
0.042 0.0050.043 0.0190.05 0.050.057 (assumed)0.06 0.060.103 0.007
SMASS = ChC
11.3011.911.98 0.3712.0012.112.15
1836 Komarov (prov. designation: 1971 OT) is a carbonaceous Dorian asteroid from the central region of the asteroid belt, approximately 22 kilometers in diameter. It was discovered on 26 July 1971 by Russian astronomer Nikolai Chernykh at Crimean Astrophysical Observatory in Nauchnij on the Crimean peninsula. It was named after Soviet cosmonaut Vladimir Komarov.
Classification and orbit
Komarov is a member of the Dora family (FIN: 512), a well-established central asteroid family of more than 1,200 carbonaceous asteroids. The family's namesake is 668 Dora. It is alternatively known as the "Zhongolovich family", named after its presumably largest member 1734 Zhongolovich. The Dora family may also contain a subfamily.13,23
It orbits the Sun at a distance of 2.3–3.3 AU once every 4 years and 8 months (1,697 days). Its orbit has an eccentricity of 0.19 and an inclination of 7° with respect to the ecliptic.
Physical characteristics
Komarov is characterized as a dark C-type asteroid by Pan-STARRS photometric survey. It is also classified as a hydrated Ch-subtype in the SMASS classification scheme.
Diameter and albedo
According to the surveys carried out by the Japanese Akari satellite and NASA's Wide-field Infrared Survey Explorer with its subsequent NEOWISE mission, Komarov measures between 21.55 and 25.40 kilometers in diameter and its surface has an albedo between 0.042 and 0.103. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous asteroids of 0.057 and calculates a diameter of 21.16 kilometers based on an absolute magnitude of 12.1.
Lightcurves
In July 2008, two rotational lightcurve of Komarov were independently obtained from photometric observations by astronomers Julian Oey and Peter Caspari. Lightcurve analysis gave a rotation period of 8.8015 and 9.695 hours with a brightness amplitude of 0.39 and 0.56 magnitude, respectively (U=3/2+).LCDB-Caspari-2008
Naming
This minor planet was named in honor of Vladimir Komarov (1927–1967), Soviet cosmonaut who headed the crewed flight on the Voskhod spacecraft. He was killed when the Soyuz 1 space capsule crashed after re-entry on 24 April 1967, due to a parachute failure.Space Exploration Reference Library 2005 Lawrence W. Baker Almanac 1 The official 1836 naming citation was published by the Minor Planet Center on 1 June 1975 (M.P.C. 3825).
Notes
LCDB-Caspari-2008 Caspari (2008): rotation period 9.695 0.005 hours with a brightness amplitude of 0.56 mag. and a quality code of 2+. Observation date:2008-07-05. Summary figures for (1836) Komarov at Collaborative Asteroid Lightcurve Link (CALL)
References
30em 2016-05-17 last obs.
JPL Small-Body Database Browser: 1836 Komarov (1971 OT)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001836
Jet Propulsion Laboratory
14 December 2016
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
147
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1837 (1836) Komarov
1836 Komarov (1971 OT)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1836
14 December 2016
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
2009
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221
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10.1007/978-3-642-01965-4
M. Broz
A. Morbidelli
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Astronomy and Astrophysics
551
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Asteroids IV
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2015aste.book..297N
10.2458/azu_uapress_9780816532131-ch016
1502.01628
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1836
14 December 2016
6
Fumihiko Usui
Daisuke Kuroda
Thomas G. Müller
Sunao Hasegawa
Masateru Ishiguro
Takafumi Ootsubo
Daisuke Ishihara
Hirokazu Kataza
Satoshi Takita
Shinki Oyabu
Munetaka Ueno
Hideo Matsuhara
Takashi Onaka
October 2011
Asteroid Catalog Using Akari: AKARI/IRC Mid-Infrared Asteroid Survey
Publications of the Astronomical Society of Japan
63
5
1117–1138
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10.1093/pasj/63.5.1117
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(online, AcuA catalog p. 153)
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NEOWISE Studies of Spectrophotometrically Classified Asteroids: Preliminary Results
The Astrophysical Journal
741
2
25
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Joseph R. Masiero
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Preliminary Analysis of WISE/NEOWISE 3-Band Cryogenic and Post-cryogenic Observations of Main Belt Asteroids
http://adsabs.harvard.edu/cgi-bin/bib_query?bibcode=2012ApJ...759L...8M
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1
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14 December 2016
Oey, Julian
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Lightcurve Analysis of Asteroids from Leura and Kingsgrove Observatory in the Second Half of 2008
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4
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1052-8091
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Mikael Granvik
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External links
Asteroid Lightcurve Database (LCDB), query form (info https://web.archive.org/web/20171216050541/http://www.minorplanet.info/lightcurvedatabase.html 16 December 2017 )
Dictionary of Minor Planet Names, Google books
Asteroids and comets rotation curves, CdR https://web.archive.org/web/20160729213840/http://obswww.unige.ch/~behrend/page_cou.html 29 July 2016 – Observatoire de Genève, Raoul Behrend
Discovery Circumstances: Numbered Minor Planets (1)-(5000) – Minor Planet Center
1836
1835 Gajdariya 1836 1837 Osita
001836
Category:Discoveries by Nikolai Chernykh
Category:Named minor planets
001836
19710726