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Vesta (minor-planet designation: 4 Vesta) is one of the largest objects in the asteroid belt, with a mean diameter of 525 kilometres (326 mi). [10]
The Vesta family (adj. Vestian; FIN: 401) is a family of asteroids. The cratering family is located in the inner asteroid belt in the vicinity of its namesake and principal body, 4 Vesta. It is one of the largest asteroid families with more than 15,000 known members and consists of mostly bright V-type asteroids, so-called "vestoids".
4 Vesta: 525.4: March 29, 1807: Dawn: 2011–2012: 210: 0.76: Dawn broke orbit on 5 September 2012 and headed to Ceres, where it arrived in March 2015: First "big four" asteroid visited by a spacecraft, largest asteroid visited by a spacecraft at the time 21 Lutetia: 120×100×80: November 15, 1852: Rosetta: 2010: 3,162: 64.9: Flyby on 10 July 2010
Claudia is a small crater that formerly defined the prime meridian of the asteroid 4 Vesta. [ b ] The convention of defining Vesta's prime meridian from Claudia is informally referred to as the Claudia coordinate system .
Veneneia / v ɛ n ɪ ˈ n iː ə / is the second-largest impact crater on asteroid 4 Vesta, at 52°S latitude. 395 kilometres (245 mi) [1] in diameter, it is 70% of the equatorial diameter of the asteroid, and one of the largest craters in the Solar System. It is at least 2 billion years old, and possibly as old as 4.2 billion years. [2]
Vibidia is an impact crater on the asteroid 4 Vesta, located at 26.9°S and 139.9°W. [2] It has a diameter of 7.1 km. [1] There is a distinctive ray-like pattern of bright and dark material, with the bright rays extending circularly for 15 km around Vibidia, and the dark rays mostly restricted to within the crater and on the rim. [3]
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Rheasilvia / ˌ r iː ə ˈ s ɪ l v i ə / is the largest impact crater on the asteroid Vesta. It is 505 km (314 mi) in diameter, which is 90% the diameter of Vesta itself, and is 95% the mean diameter of Vesta, 529 km (329 mi). However, the mean is affected by the crater itself.