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1837 Osita
Reference material by Wikipedia contributors. This retains its source identity and is not 411 news reporting.
Stony main-belt asteroid
October 2019
yes
1837 Osita
#D6D6D6
001837-asteroid shape model (1837) Osita.png
Shape model of Osita from its lightcurve
16 August 1971
J. Gibson
El Leoncito Complex
(1837) Osita
1971 QZ 11962 XQ1968 QB 11972 YJ 1
Ursula Gibson(astronomer's wife)
main-beltFlora
4 September 2017 (JD 2458000.5)
0
54.27 yr (19,823 days)
2.3955 AU
2.0158 AU
2.2057 AU
0.0861
3.28 yr (1,196 days)
93.913°
0.3009 ms / day
3.8455°
280.93°
315.11°
7.14 km (calculated)7.530 0.1197.693 0.061 km7.85 0.29 km7.94 0.58 km
3.8186 0.0020 h3.81862 0.0001 3.81880 0.00005 h
0.194 0.0300.198 0.0240.2067 0.02540.216 0.0190.24 (assumed)
AQS
12.674 0.001 (R)12.81 0.2312.9
1837 Osita (prov. designation: 1971 QZ 1) is a stony Flora asteroid from the inner regions of the asteroid belt, approximately 7 kilometers in diameter. It was discovered on 16 August 1971, by American astronomer James Gibson at the Yale–Columbia Southern Station of the Leoncito Astronomical Complex in Argentina, who named it after his wife Ursula ("Osita").
Orbit and classification
The S-type asteroid is a member of the Flora family, one of the largest groups of stony asteroids in the main-belt. It orbits the Sun in the inner main-belt at a distance of 2.0–2.4 AU once every 3 years and 3 months (1,196 days). Its orbit has an eccentricity of 0.09 and an inclination of 4° with respect to the ecliptic. Osita was first identified as 1962 XQ at Goethe Link Observatory in 1962, extending the body's observation arc by 9 years prior to its official discovery observation.
Physical characteristics
PanSTARRSs large-scale survey also classified Osita as a rare AQ-type, having intermediate spectral characteristics of an A and Q type asteroid.
Rotation period
In February 2006, a rotational lightcurve of Osita was obtained from photometric observation by French amateur astronomer René Roy, giving a well-defined rotation period of 3.81880 hours with a brightness variation of 0.48 magnitude (U=3). Photometric observations in the R-band at the Palomar Transient Factory in October 2011, gave a concurring period of 3.8186 hours and an amplitude of 0.59 magnitude (U=2). A third period of 3.81880 hours was derived from a large international data-mining collaboration in February 2016 (U=n.a.).
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, Osita measures between 7.53 and 7.94 kilometers in diameter, and its surface has an albedo between 0.194 and 0.216.
The Collaborative Asteroid Lightcurve Link assumes an albedo of 0.24 – derived from 8 Flora, the largest member and namesake of this orbital family – and calculates a diameter of 7.14 kilometers with an absolute magnitude of 12.9.
Naming
This minor planet was named by the discoverer for his wife Ursula ("Osita" is the Spanish equivalent). She volunteered as an assistant and actively participated in the observations by measuring or reducing more than 150 positions of comets and minor planets. The official 1837 naming citation was published by the Minor Planet Center on 20 February 1976 (M.P.C. 3935).
References
30em 2017-03-11 last obs.
JPL Small-Body Database Browser: 1837 Osita (1971 QZ1)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001837
Jet Propulsion Laboratory
8 June 2017
Dictionary of Minor Planet Names – (1837) Osita
Schmadel Lutz D.
Springer Berlin Heidelberg
147
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1838 (1837) Osita
1837 Osita (1971 QZ1)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1837
14 December 2016
Dictionary of Minor Planet Names – Addendum to Fifth Edition (2006–2008)
Appendix – Publication Dates of the MPCs
Schmadel Lutz D.
Springer Berlin Heidelberg
221
978-3-642-01964-7
10.1007/978-3-642-01965-4
Asteroids and comets rotation curves – (1837) Osita
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001837
14 December 2016
1 April 2019
https://web.archive.org/web/20190401181659/http://obswww.unige.ch/~behrend/page4cou.html#001837
dead
1837
14 December 2016
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The Astrophysical Journal Letters
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M. Audejean
P. Aurard
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L. Bernasconi
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I. Bozhinova
J. Brinsfield
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G. Casalnuovo
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G. Dubos
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R. Dymock
A. Escalante del Valle
N. Esseiva
R. Esseiva
M. Esteban
T. Fauchez
M. Fauerbach
M. Fauvaud
S. Fauvaud
E. Forné
C. Fournel
D. Fradet
J. Garlitz
O. Gerteis
C. Gillier
M. Gillon
R. Giraud
J.-P. Godard
R. Goncalves
Hiroko Hamanowa
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K. Hay
S. Hellmich
S. Heterier
D. Higgins
R. Hirsch
G. Hodosan
M. Hren
A. Hygate
N. Innocent
H. Jacquinot
S. Jawahar
E. Jehin
L. Jerosimic
A. Klotz
W. Koff
P. Korlevic
E. Kosturkiewicz
P. Krafft
Y. Krugly
F. Kugel
O. Labrevoir
J. Lecacheux
M. Lehký
A. Leroy
B. Lesquerbault
M. J. Lopez-Gonzales
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B. Mallecot
J. Manfroid
F. Manzini
A. Marciniak
A. Martin
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F. Reignier
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D. Robilliard
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A. Scholz
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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
1837
1836 Komarov 1837 1838 Ursa
001837
Category:Discoveries by James B. Gibson (astronomer)
Category:Named minor planets
19710816