On the transport of bodies within and from the asteroid belt
作者： Fred Franklin , Myron Lecar
DOI: 10.1111/J.1945-5100.2000.TB01778.X
关键词: Asteroid belt 、 Formation and evolution of the Solar System 、 Drag 、 Parent body 、 Nebula 、 Geology 、 Secular resonance 、 Solar System 、 Astronomical unit 、 Astronomy
摘要: — This paper explores two processes, sweeping secular resonance (Ward, 1981) and gas drag (Lecar Franklin, 1997), at work during the dispersal of solar nebula. we have aims not previously considered for mechanisms: (1) to explain likely depletion, by a factor 1000 or so, rocky material in inner belt (2.0 3.3 AU) well into one, that an object already as large even larger than Vesta (r = 250 km)—thought be parent body many meteorites—can inwardly displaced much astronomical unit if nebula times lie close 105 years. For such times, fraction belt's primordial mass can ejected, with most it passing system.
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