Vesta is the second most massive body in the asteroid belt, surpassed only by Ceres, which is classified as a dwarf planet. The brightest asteroid in the sky, Vesta is occasionally visible from Earth with the naked eye. It is the first of the four largest asteroids Ceres, Vesta, Pallas and Hygiea to be visited by a spacecraft. The Dawn mission orbited Vesta in , providing new insights into this rocky world. In , while determining the elliptical shape of planetary orbits, Johannes Kepler came to believe that a planet should exist in the gap between Mars and Jupiter. Mathematical calculations by Johann Daniel Titius and Johann Elert Bode in — later known as the Titius-Bode law — seemed to support this prediction.
Physical characteristics of Vesta
Vesta is the second-largest asteroid, both by mass and by volume, after the dwarf planet Ceres. Vesta is the only known remaining rocky protoplanet with a differentiated interior of the kind that formed the terrestrial planets. Vesta is the brightest asteroid visible from Earth. Its maximum distance from the Sun is slightly greater than the minimum distance of Ceres from the Sun, [d] though its orbit lies entirely within that of Ceres. NASA's Dawn spacecraft entered orbit around Vesta on 16 July for a one-year exploration and left orbit on 5 September  en route to its final destination, Ceres. Researchers continue to examine data collected by Dawn for additional insights into the formation and history of Vesta. Heinrich Olbers discovered Pallas in , the year after the discovery of Ceres. He proposed that the two objects were the remnants of a destroyed planet. He sent a letter with his proposal to the British astronomer William Herschel , suggesting that a search near the locations where the orbits of Ceres and Pallas intersected might reveal more fragments.
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