(39529) Vatnajokull
Asteroid (39529) Vatnajokull |
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Properties of the orbit ( animation ) | |
Orbit type | Inner main belt asteroid |
Major semi-axis | 2.3267 AU |
eccentricity | 0.1448 |
Perihelion - aphelion | 1.9897 AU - 2.6637 AU |
Inclination of the orbit plane | 8.0501 ° |
Length of the ascending node | 177.9136 ° |
Argument of the periapsis | 203.5441 ° |
Sidereal period | 3.55 a |
Physical Properties | |
Absolute brightness | 15.8 mag |
history | |
Explorer | Eric Walter Elst |
Date of discovery | 3rd November 1989 |
Another name | 1989 VJ 1 , 1996 TX 37 |
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. |
(39529) Vatnajökull is an asteroid of the main inner belt , which was discovered on November 3, 1989 by the Belgian astronomer Eric Walter Elst at the La Silla Observatory of the European Southern Observatory in Chile ( IAU code 809).
Mean distance from the Sun ( major semiaxis ), eccentricity and inclination of the orbit plane of the asteroid correspond roughly 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. According to the SMASS classification ( Small Main-Belt Asteroid Spectroscopic Survey ), a spectroscopic study by Gianluca Masi , Sergio Foglia and Richard P. Binzel at (39529) Vatnajökull assumed a bright surface, so it could be roughly seen be an S asteroid , not a V asteroid.
(39529) Vatnajökull was named on October 8, 2014 after Vatnajökull , the largest glacier in Iceland .
See also
Web links
- (39529) Vatnajökull in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- (39529) Vatnajökull in the Small-Body Database of the Jet Propulsion Laboratory (English).
- Discovery Circumstances of (39529) Vatnajökull according to the Minor Planet Center of the International Astronomical Union at the Harvard-Smithsonian Center for Astrophysics in Cambridge , Massachusetts (English)
Individual evidence
- ^ Gianluca Masi, Sergio Foglia, Richard P. Binzel: Search for Unusual Spectroscopic Candidates Among 40313 minor planets from the 3rd Release of the Sloan Digital Sky Survey Moving Object Catalog . (English)
- ↑ subdivision of asteroids to S-types, C-types and V-types (English)