(4928) Vermeer
| Asteroid (4928) Vermeer | |
|---|---|
| Properties of the orbit ( animation ) | |
| Orbit type | Inner main belt asteroid | 
| Major semi-axis | 2.1473 AU | 
| eccentricity | 0.1891 | 
| Perihelion - aphelion | 1.7412 AU - 2.5535 AU | 
| Inclination of the orbit plane | 2.4580 ° | 
| Length of the ascending node | 207.6043 ° | 
| Argument of the periapsis | 131.4371 ° | 
| Sidereal period | 3.15 a | 
| Mean orbital velocity | 20.32 km / s | 
| Physical Properties | |
| Rotation period | 3.687 h (± 0.001) | 
| Absolute brightness | 14.2 mag | 
| history | |
| Explorer | Lyudmila Georgievna Karachkina | 
| Date of discovery | October 12, 1982 | 
| Another name | 1982 UG 7 , 1982 XR 3 | 
| 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. | |
(4928) Vermeer is an asteroid of the main inner belt , which was discovered by the Soviet astronomer Lyudmila Georgievna Karachkina on October 12, 1982 at the Crimean Observatory in Nautschnyj ( IAU code 095).
The asteroid's period of rotation was measured for the first time on September 9 and 10, 2010, at the Osservatorio astronomico della Regione Autonoma Valle d'Aosta in Nus -Saint-Barthélemy by the Italian astronomer Albino Carbognani with an 81 cm Ritchey-Chrétien-Cassegrain Telescope , and determined to be 3.687 (± 0.003) hours. Due to the short rotation period and the two long observation times, (4928) Vermeer could be used as a test object for the method of redshift measurement in 17 other asteroids.
The asteroid was on 1 September 1993 by Jan Vermeer designated to one of the most famous Dutch painter of the Baroque is.
Web links
- (4928) Vermeer in the database of the "Asteroids - Dynamic Site" (AstDyS-2, English).
- (4928) Vermeer in the Small-Body Database of the Jet Propulsion Laboratory of NASA at the California Institute of Technology (Caltech) in Pasadena , California (English)
Individual evidence
- ^ Albino Carbognani: Lightcurves and Periods of Eighteen NEAs and MBAs . The Minor Planet Bulletin, vol. 38, no. 1, 01/2011, pages 57 to 60, bibcode : 2011MPBu ... 38 ... 57C . (English)
- ^ Lutz D. Schmadel : Dictionary of Minor Planet Names . Springer, Heidelberg 2003, 5th edition, page 425 (English)
