(9329) Nikolaimedtner
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Asteroid (9329) Nikolaimedtner |
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| Properties of the orbit ( animation ) | |
| Orbit type | Main belt asteroid |
| Asteroid family | Vesta family |
| Major semi-axis | 2.2893 AU |
| eccentricity | 0.0906 |
| Perihelion - aphelion | 2.0820 AU - 2.4966 AU |
| Inclination of the orbit plane | 5.9808 ° |
| Length of the ascending node | 243.8223 ° |
| Argument of the periapsis | 21.3314 ° |
| Sidereal period | 3.46 a |
| Mean orbital velocity | 19.68 km / s |
| Physical Properties | |
| Absolute brightness | 13.9 likes |
| history | |
| Explorer | Eric Walter Elst |
| Date of discovery | March 2, 1990 |
| Another name | 1990 EO , 1991 PG 12 |
| Source: Unless otherwise stated, the data comes from JPL Small-Body Database Browser . The affiliation to an asteroid family is automatically determined from the AstDyS-2 database . Please also note the note on asteroid items. | |
(9329) Nikolaimedtner is an asteroid of the main belt , which on 2 March 1990 by the Belgian astronomer Eric Walter Elst at the La Silla Observatory of the European Southern Observatory in Chile ( IAU code was discovered 809).
The asteroid belongs to the Vesta family , a large group of asteroids named after (4) Vesta , the second largest asteroid and third largest celestial body in the main belt.
(9329) Nikolaimedtner was named on March 18, 2003 after the Russian composer and pianist Nikolai Karlowitsch Medtner (1880–1951) who, together with Alexander Konstantinowitsch Glasunow , Paul Juon and Sergei Iwanowitsch Taneyev, stamped the label of a "Russian Brahms" on because they combined elements of the national Russian school with Western European influences.
See also
Web links
- (9329) Nikolaimedtner in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- (9329) Nikolaimedtner in the Small-Body Database of the Jet Propulsion Laboratory of NASA at the California Institute of Technology (Caltech) in Pasadena , California (English)
- Discovery Circumstances by (9329) Nikolaimedtner according to the Minor Planet Center of the International Astronomical Union at the Harvard-Smithsonian Center for Astrophysics in Cambridge , Massachusetts (English)
Individual evidence
- ↑ The family status of the asteroids in the AstDyS-2 database (English, HTML; 51.4 MB)