Vesta, the brightest asteroid of all, revolves around the Sun in 3.6 terrestrial years and its mean diameter is about 520 km. This huge rock of irregular shape, with no trace of water, has a core composed of iron. The enormous crater at the south pole of Vesta is 460 km wide and 13 km deep. This is the result of a massive collision appears to have torn part of the small planet. Astronomers believe that 5% of meteorites found on Earth come from this huge shock. In July 2011, the Dawn spacecraft to Vesta has come to stay in orbit a year or so and then turn back on its engines to reach a much larger asteroid, Ceres, it will reach in 2015. The journey of the probe Dawn ("Dawn" in English) will enlighten us a little about the birth of our solar system and on planet formation. Dawn will travel a total of 5.1 billion km, 7 months evolve around each asteroid.
Overflights at low altitude are planned, at an altitude of 15 km to Vesta and Ceres to 40 km.
Vesta (4) | ||
dimensions | 578 × 560 × 458 km | |
Rotation period | 5,342 ours | |
Density | 3,4 g/cm3 | |
Aphelion | 384,920740×106 km (2,573034 ua) | |
Perihelion | 321,767047×106 km (2,150878 ua) | |
Mass | 2,7 × 1020 kg | |
Esscape speed | 0,18 km/s | |
Discovered | 29 mars 1807 |
The first pictures of the probe descends Vesta Dawn since July 16, 2011 to 5200 km, it already reveals some curiosities. The landscape is riddled with craters Earth surprising, in fact, the asteroid is heavily cratered 530 km in its northern part, while its southern part is quite smooth. The number of craters is very surprising because the density of craters, has not been observed elsewhere, on other planets.
Over long parallel scratches are around Vesta.
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