caa a22 4500 445816201 CHVBK 20180317145229.0 cr unu---uuuuu 170323e20111201xx s 000 0 eng 10.1007/s11214-011-9792-x doi (NATIONALLICENCE)springer-10.1007/s11214-011-9792-x Vesta and Ceres: Crossing the History of the Solar System [Elektronische Daten] [A. Coradini, D. Turrini, C. Federico, G. Magni] The evolution of the Solar System can be schematically divided into three different phases: the Solar Nebula, the Primordial Solar System and the Modern Solar System. These three periods were characterized by very different conditions, both from the point of view of the physical conditions and from that of the processes there were acting through them. Across the Solar Nebula phase, planetesimals and planetary embryos were forming and differentiating due to the decay of short-lived radionuclides. At the same time, giant planets formed their cores and accreted the nebular gas to reach their present masses. After the gas dispersal, the Primordial Solar System began its evolution. In the inner Solar System, planetary embryos formed the terrestrial planets and, in combination with the gravitational perturbations of the giant planets, depleted the residual population of planetesimals. In the outer Solar System, giant planets underwent a violent, chaotic phase of orbital rearrangement which caused the Late Heavy Bombardment. Then the rapid and fierce evolution of the young Solar System left place to the more regular secular evolution of the Modern Solar System. Vesta, through its connection with HED meteorites, and plausibly Ceres too were between the first bodies to form in the history of the Solar System. Here we discuss the timescale of their formation and evolution and how they would have been affected by their passage through the different phases of the history of the Solar System, in order to draw a reference framework to interpret the data that Dawn mission will supply on them. Springer Science+Business Media B.V., 2011 Asteroid Vesta nationallicence Asteroid Ceres nationallicence Asteroids nationallicence Meteorites nationallicence Solar system formation nationallicence Solar system evolution nationallicence Impacts nationallicence Coradini A. Institute for Physics of Interplanetary Space, INAF, Rome, Italy aut Turrini D. Institute for Physics of Interplanetary Space, INAF, Rome, Italy aut Federico C. Department of Earth Sciences, University of Perugia, Perugia, Italy aut Magni G. Institute for Space Astrophysics and Cosmic Physics, INAF, Rome, Italy aut Space Science Reviews Springer Netherlands 163/1-4(2011-12-01), 25-40 0038-6308 163:1-4<25 2011 163 11214 https://doi.org/10.1007/s11214-011-9792-x text/html Onlinezugriff via DOI 1 review-article jats NATIONALLICENCE 856 40 https://doi.org/10.1007/s11214-011-9792-x text/html Onlinezugriff via DOI NATIONALLICENCE 700 1- Coradini A. Institute for Physics of Interplanetary Space, INAF, Rome, Italy aut NATIONALLICENCE 700 1- Turrini D. Institute for Physics of Interplanetary Space, INAF, Rome, Italy aut NATIONALLICENCE 700 1- Federico C. Department of Earth Sciences, University of Perugia, Perugia, Italy aut NATIONALLICENCE 700 1- Magni G. Institute for Space Astrophysics and Cosmic Physics, INAF, Rome, Italy aut NATIONALLICENCE 773 0- Space Science Reviews Springer Netherlands 163/1-4(2011-12-01), 25-40 0038-6308 163:1-4<25 2011 163 11214 Metadata rights reserved Springer special CC-BY-NC licence nationallicence BK010053 XK010053 XK010000 NATIONALLICENCE NATIONALLICENCE NL-springer