(5063) Monteverdi
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Asteroid (5063) Monteverdi |
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|---|---|
| Properties of the orbit ( animation ) | |
| Orbit type | Main belt |
| Asteroid family | Hertha family |
| Major semi-axis | 2.3923 AU |
| eccentricity | 0.2273 |
| Perihelion - aphelion | 1.8486 AU - 2.9360 AU |
| Inclination of the orbit plane | 1.5371 ° |
| Length of the ascending node | 326.6840 ° |
| Argument of the periapsis | 56.1021 ° |
| Sidereal period | 3.70 a |
| Mean orbital velocity | 19.26 km / s |
| Physical Properties | |
| Absolute brightness | 13.9 likes |
| history | |
| Explorer | Freimut Börngen |
| Date of discovery | February 2, 1989 |
| Another name | 1989 CJ 5 , 1954 SK, 1991 RU 1 |
| 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. | |
(5063) Monteverdi is an asteroid of the main belt that was discovered on February 2, 1989 by the German astronomer Freimut Börngen at the Thuringian state observatory in Tautenburg ( IAU code 033) in Thuringia .
The asteroid belongs to the Nysa group, a group of asteroids named after (44) Nysa (also called the Hertha family, after (135) Hertha ).
(5063) Monteverdi was named after the Italian composer , gambist , singer and Catholic priest Claudio Monteverdi (1567–1643), whose work accompanied the transition from Renaissance to Baroque music and who was probably the first to compose operas on a large scale .
See also
Individual evidence
- ↑ The family membership of (5063) Monteverdi in the AstDyS-2 database (English)
Web links
- Asteroid Monteverdi: Discovery Circumstances according to the Minor Planet Center of the International Astronomical Union at the Harvard-Smithsonian Center for Astrophysics, Cambridge, USA
- Asteroid Monteverdi in the Small-Body Database of the Jet Propulsion Laboratory of NASA at the California Institute of Technology, Pasadena, USA
- (5063) Monteverdi in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).