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1799 Koussevitzky
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Main-belt asteroid
December 2018
yes
1799 Koussevitzky
#D6D6D6
001799-asteroid shape model (1799) Koussevitzky.png
Koussevitzky modeled from its lightcurve
Indiana University(Indiana Asteroid Program)
Goethe Link Obs.
25 July 1950
(1799) Koussevitzky
1950 OE1929 QD1974 CF 1
Serge Koussevitzky(Russian conductor)
main-belt(outer)Eosbackground
27 April 2019 (JD 2458600.5)
0
68.24 yr (24,926 d)
3.3845 AU
2.6690 AU
3.0267 AU
0.1182
5.27 yr (1,923 d)
359.04°
0.1872 ms / day
11.489°
156.61°
193.02°
17.88 1.23 km18.196 0.156 km19.067 0.298 km23.26 2.4 km
6.318 0.005 hlightcurve-plot-Warner
0.14260.21280.2330.241
SMASS KL
10.9011.311.59 0.29
1799 Koussevitzky (prov. designation: 1950 OE) is an asteroid of the Eos family from the outer regions of the asteroid belt, approximately 18 km mi off 2 us in diameter. It was discovered on 25 July 1950, by astronomers at Indiana University during the Indiana Asteroid Program at Goethe Link Observatory in Indiana, United States. The K-type asteroid has a rotation period of 6.3 hours. It was named for Russian conductor Serge Koussevitzky.
Orbit and classification
According to several HCM-analyses by Zappalà, Mothé-Diniz, as well as Milani and Knežević, Koussevitzky is a core member the Eos family (606), the largest asteroid family of the outer main belt consisting of nearly 10,000 asteroids. However, in a more recent HCM-analysis by Nesvorný, Koussevitzky is a non-family asteroid from the main belt's background population.
It orbits the Sun in the outer asteroid belt at a distance of 2.7–3.4 AU once every 5 years and 3 months (1,923 days; semi-major axis of 3.03 AU). Its orbit has an eccentricity of 0.12 and an inclination of 11° with respect to the ecliptic. The asteroid was first observed as 1929 QD at Simeiz Observatory in August 1929. The body's observation arc begins with its official discovery observation at Goethe Link in July 1950.
Naming
This minor planet was named in memory of Russian-born Serge Koussevitzky (1874–1951), long-time music director and conductor of the Boston Symphony Orchestra. The asteroid's name was proposed by astronomer Frank K. Edmondson of Indiana University on the occasion of Serge Koussevitzky's centenary of the birth on 26 July 1974. The official 1799 naming citation was published by the Minor Planet Center on 1 January 1974 (M.P.C. 3569).
Physical characteristics
In the SMASS classification, Koussevitzky is a stony K-type asteroid, typical for members of the Eos family. The asteroid has also been characterized as an L-type by Pan-STARRS.
Rotation period
In June 2013, a rotational lightcurve of Koussevitzky was obtained from photometric observations by Brian Warner at the Palmer Divide Station U82 in California. Lightcurve analysis gave a well-defined rotation period of 6.318 0.005 hours with a brightness variation of 0.40 magnitude (U=3).lightcurve-plot-Warner Alternative period determinations of 6.325, 6.328 and 6.329 hours were made by astronomers at the University of Iowa using its Rigel Telescope at the Iowa Robotic Observatory 857 in Arizona, by French amateur astronomer René Roy, and by staff members of the Palomar Transient Factory in California, respectively (U=x2/3-/2).
Diameter and albedo
According to the surveys carried out by the Infrared Astronomical Satellite IRAS, the Japanese Akari satellite and the NEOWISE mission of NASA's Wide-field Infrared Survey Explorer, Koussevitzky measures between 17.88 and 23.26 kilometers in diameter and its surface has an albedo between 0.1426 and 0.241. The Collaborative Asteroid Lightcurve Link derives an albedo of 0.1506 and a diameter of 18.82 kilometers based on an absolute magnitude of 11.3.
Notes
lightcurve-plot-Warner Lightcurve plot of (1799) Koussevitzky, B. Warner, June 2013, rotation period 6.318 0.005 hours with a brightness amplitude of 0.4 mag. Quality code is 3 (at CS3). Summary figures at the LCDB and CS3.
References
30em 2018-10-22 last obs.
JPL Small-Body Database Browser: 1799 Koussevitzky (1950 OE)
https://ssd.jpl.nasa.gov/sbdb.cgi?sstr=2001799
Jet Propulsion Laboratory
10 December 2018
Dictionary of Minor Planet Names – (1799) Koussevitzky
Schmadel Lutz D.
Springer Berlin Heidelberg
144
2007
978-3-540-00238-3
10.1007/978-3-540-29925-7_1800 (1799) Koussevitzky
1799 Koussevitzky (1950 OE)
Minor Planet Center
https://www.minorplanetcenter.net/db_search/show_object?object_id=1799
10 December 2018
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 2009
https://cds.cern.ch/record/1339661
Asteroids and comets rotation curves – (1799) Koussevitzky
Behrend
Raoul
Geneva Observatory
http://obswww.unige.ch/~behrend/page4cou.html#001799
10 December 2018
1 April 2019
https://web.archive.org/web/20190401181659/http://obswww.unige.ch/~behrend/page4cou.html#001799
dead
Asteroid (1799) Koussevitzky – Proper elements
AstDyS-2, Asteroids – Dynamic Site
https://newton.spacedys.com/astdys/index.php?n=1799&pc=1.1.6
4 December 2018
Asteroid 1799 Koussevitzky
Small Bodies Data Ferret
https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1799+Koussevitzky
10 December 2018
https://web.archive.org/web/20181210202738/https://sbntools.psi.edu/ferret/SimpleSearch/results.action?targetName=1799+Koussevitzky
10 December 2018
dead
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NASA Planetary Data System – IRAS-A-FPA-3-RDR-IMPS-V6.0
IRAS–A–FPA–3–RDR–IMPS–V6.0
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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
1799
1798 Watts 1799 1800 Aguilar
001799
001799
001799
Category:Named minor planets
001799
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