(2347) Vinata
Asteroid (2347) Vinata |
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Properties of the orbit ( animation ) | |
Orbit type | Main outer belt asteroid |
Major semi-axis | 3.0895 AU |
eccentricity | 0.2130 |
Perihelion - aphelion | 2.4313 AU - 3.7477 AU |
Inclination of the orbit plane | 13.0826 ° |
Length of the ascending node | 290.4593 ° |
Argument of the periapsis | 108.3677 ° |
Time of passage of the perihelion | 5th August 2018 |
Sidereal period | 5.43 a |
Mean orbital velocity | 16.94 km / s |
Physical Properties | |
Medium diameter | 25.398 km (± 0.332) |
Albedo | 0.083 (± 0.009) |
Rotation period | 4.4835 h (± 0.0005) |
Absolute brightness | 11.3 mag |
history | |
Explorer | Henry Lee Giclas |
Date of discovery | October 7, 1936 |
Another name | 1936 TK , 1976 EG, 1979 PC |
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. |
(2347) Vinata is an asteroid of the outer main belt , which the US American astronomer Henry Lee Giclas on October 7, 1936 at the Lowell Observatory ( IAU code 690) in Flagstaff , Arizona was discovered.
The mean diameter of the asteroid was calculated to be around 25 kilometers.
The asteroid's period of rotation was observed on December 13-16, 2007 by Brian D. Warner at the Palmer Divide Observatory in Colorado . The light curve gave a rotation period of 4.4835 h (± 0.0005).
(2347) Vinata was named after Vinata on February 6, 1993 at the suggestion of the American astronomer Frederick Pilcher , the mother of Aruna and Garuda in Indian mythology . The asteroids (2313) Aruna and (2307) Garuda were named after Aruna and Garuda on the same day .
Web links
- (2347) Vinata in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- (2347) Vinata 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 of (2347) Vinata according to the Minor Planet Center of the International Astronomical Union at the Harvard-Smithsonian Center for Astrophysics in Cambridge , Massachusetts (English)
Individual evidence
- ↑ Brian D. Warner: ASTEROID LIGHTCURVE ANALYSIS AT THE PALMER DIVIDE OBSERVATORY: SEPTEMBER-DECEMBER 2007 . The Minor Planet Bulletin, Vol. 35, pages 67 and 69, 2008 ( PDF , 662 kB; English)