(43775) Tiepolo
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Asteroid (43775) Tiepolo |
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| Properties of the orbit ( animation ) | |
| Orbit type | Main outer belt asteroid |
| Asteroid family | Ursula family |
| Major semi-axis | 3.1632 AU |
| eccentricity | 0.1127 |
| Perihelion - aphelion | 2.8066 AU - 3.5197 AU |
| Inclination of the orbit plane | 16.1787 ° |
| Length of the ascending node | 321.4254 ° |
| Argument of the periapsis | 233.6286 ° |
| Time of passage of the perihelion | January 9, 2018 |
| Sidereal period | 5.63 a |
| Mean orbital velocity | 16.74 km / s |
| Physical Properties | |
| Medium diameter | 10.840 (± 0.221) km |
| Albedo | 0.104 (± 0.023) |
| Absolute brightness | 13.5 likes |
| history | |
| Explorer | Freimut Börngen |
| Date of discovery | February 2, 1989 |
| Another name | 1989 CA 6 , 1999 XX 205 |
| 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. | |
(43775) Tiepolo is an asteroid of the outer main belt that was discovered by the German astronomer Freimut Börngen on February 2, 1989 at the Karl Schwarzschild Observatory ( IAU code 033) in the Tautenburg Forest .
The mean diameter of the asteroid was calculated to be 10.840 (± 0.221) kilometers and the albedo to be 0.104 (± 0.023).
The asteroid belongs to the Ursula family, a several billion year old asteroid family named after the asteroid (375) Ursula .
The track from (43775) Tiepolo was secured in 2002 so that numbering could be assigned. On January 6, 2003, the asteroid was named after Giovanni Battista Tiepolo (1696-1770) at the suggestion of Freimut Börngen . Tiepolo was one of the most important Venetian painters of the late Baroque and Rococo .
See also
Web links
- (43775) Tiepolo in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- (43775) Tiepolo in the Small-Body Database of the Jet Propulsion Laboratory .
- Discovery Circumstances of (43775) Tiepolo 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)
- ↑ Valerio Carruba, David Nesvorný , Safwan Aljbaae, Rita de Cássia Domingos, Mariela Huaman Espinoza: On the oldest asteroid families in the main belt . Monthly Notes of the Royal Astronomical Society, March 3, 2016 ( PDF ; 1.422 MB)
- ↑ Small planets discovered on Tautenburger Platten on the website of Freimut Börngen