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1180 Rita
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Main-belt asteroid
December 2019
yes
1180 Rita
#D6D6D6
9 April 1931
K. Reinmuth
Heidelberg Obs.
(1180) Rita
1931 GE1929 CM1953 AH1957 UF 1A907 GGA908 KAA916 LA
unknown
main-belt(outer)Hilda
16 February 2017 (JD 2457800.5)
0
109.98 yr (40,172 days)
4.6127 AU
3.3574 AU
3.9851 AU
0.1575
7.96 yr (2,906 days)
209.15°
0.1239 ms / day
7.1985°
88.336°
209.12°
0.6111 AU
82.72 km (calculated)97 km97.63 2.30 km
9 h9.605 0.006 h12 h13.090 0.002 hLCDB-Warner-201714.72 h14.902 h20.496 0.005 hLCDB-Slyusarev-2012
0.041 0.0020.044 0.0080.0480.057 (assumed)0.058 0.009
Tholen = PPB–V 0.6820.670 0.010LCDB-Slyusarev-2012U–B = 0.216V–R = 0.440 0.010LCDB-Slyusarev-2012
9.149.17 0.19
1180 Rita, provisional designation 1931 GE, is a dark and spheroidal Hildian asteroid from the outermost regions of the asteroid belt, approximately 97 kilometers in diameter. It was discovered on 9 April 1931, by German astronomer Karl Reinmuth at the Heidelberg Observatory in southwest Germany. Any reference of its later name, Rita, is unknown.
Orbit and classification
Rita belongs to the orbital Hilda group which is located in the outermost part of the main-belt. Asteroids in this dynamical group have semi-major axis between 3.7 and 4.2 AU and stay in a 3:2 resonance with the gas giant Jupiter. Rita, however, is a background asteroid and not a member of the (collisional) Hilda family (101). Hildian asteroids are thought to have originated from the Kuiper belt.
The asteroid orbits the Sun at a distance of 3.4–4.6 AU once every 7 years and 12 months (2,906 days). Its orbit has an eccentricity of 0.16 and an inclination of 7° with respect to the ecliptic.
It was first observed as A907 GG at Heidelberg in 1907. The body's observation arc begins at Heidelberg in 1908, when it was identified as A908 KA, approximately 23 years prior to its official discovery observation.
Physical characteristics
In the Tholen taxonomy, Rita is a dark and reddish P-type asteroid. The P-type asteroids are some of the darkest objects in the Solar System.
Rotation period
Since 1983, several rotational lightcurves of Rita have been obtained from photometric observations. Lightcurve analysis gave a wide range of divergent rotation periods between 9 and 20.5 hours.LCDB-Slyusarev-2012 The Light Curve Data Base adopts a period of 13.090 hours with a brightness amplitude of 0.06 magnitude. Bodies with such a low brightness variation are typically of a spherical rather than elongated shape. The lightcurve was obtained in January 2017, by American astronomer Brian Warner at the Center for Solar System Studies in California (U=2).LCDB-Warner-2017
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, Rita measures 97 kilometers in diameter and its surface has an albedo between 0.041 and 0.058. The Collaborative Asteroid Lightcurve Link assumes a standard albedo for carbonaceous, outer main-belt asteroids of 0.057, and calculates a diameter of 82.72 kilometers with on an absolute magnitude of 9.14.
Naming
Any reference of this minor planet's name to a person or occurrence is unknown.
Unknown meaning
Among the many thousands of named minor planets, Rita is one of 120 asteroids, for which no official naming citation has been published. All of these low-numbered asteroids have numbers between 164 164 Eva and 1514 1514 Ricouxa and were discovered between 1876 and the 1930s, predominantly by astronomers Auguste Charlois, Johann Palisa, Max Wolf and Karl Reinmuth.
Notes
LCDB-Warner-2017 Warner (2017) web: lightcurve plot of 1180 Rita – rotation period 13.090 0.002 hours with a brightness amplitude of 0.06 0.01 magnitude. No quality code of 2. Observed between 12 December 2016 and 26 January 2017, with a total of 304 data points. Summary figures at the Light Curve Data Base.
LCDB-Slyusarev-2012 Slyusarev (2012) web: rotation period 20.496 0.005 hours with a brightness amplitude of 0.05 magnitude. No quality code determined. Color Indices for BV and VR are 0.670 0.010 and 0.440 0.010, respectively. Summary figures at the Light Curve Data Base.
References
30em 2017-03-29 last obs.
JPL Small-Body Database Browser: 1180 Rita (1931 GE)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001180
Jet Propulsion Laboratory
27 April 2017
Schmadel Lutz D.
Dictionary of Minor Planet Names Springer Berlin Heidelberg
99
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1181 (1180) Rita
Dictionary of Minor Planet Names – Fifth Revised and Enlarged revision
Appendix 11 – Minor Planet Names with Unknown Meaning
Schmadel Lutz D.
Springer Berlin Heidelberg
927–929
2007
978-3-540-00238-3
Lutz D. Schmadel
1180 Rita (1931 GE)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1180
27 April 2017
Asteroids and comets rotation curves – (1180) Rita
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page3cou.html#001180
27 April 2017
3 December 2002
https://web.archive.org/web/20021203214643/http://obswww.unige.ch/~behrend/page3cou.html#001180
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Asteroid 1180 Rita – Proper Elements
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https://newton.spacedys.com/astdys/index.php?pc=1.1.6&n=1180
28 October 2019
1180
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27 April 2017
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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
1180
1179 Mally 1180 1181 Lilith
001180
Category:Discoveries by Karl Wilhelm Reinmuth
Category:Named minor planets
001180
19310409