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Growth and Evolution of Asteroids
被引:75
|作者:
Asphaug, Erik
[1
]
机构:
[1] Univ Calif Santa Cruz, Dept Earth & Planetary Sci, Santa Cruz, CA 95064 USA
关键词:
planet formation;
planetesimals;
small bodies;
accretion;
NEOs;
KUIPER-BELT OBJECTS;
MAIN-BELT;
433;
EROS;
RADAR OBSERVATIONS;
EARTH;
YARKOVSKY;
BREAKUP;
IMPACT;
VESTA;
POPULATION;
D O I:
10.1146/annurev.earth.36.031207.124214
中图分类号:
P1 [天文学];
学科分类号:
0704 ;
摘要:
Asteroids are what is left of the precursors to the terrestrial planets. They are stunning ill their diversity, ranging from charcoal-black worlds the size, of a hilltop, spinning like a carnival ride, to dog-bone-shaped metallic remnants of some cataclysmically disrupted planetary core, to worlds as stately as Ceres and Vesta (and fragments thereof), to garden-variety fractured and blocky nuggets that dominate near-Earth space. Asteroid belts are common around Sun-like stars. When properly seen as unaccreted residues, as scraps on the floor of the planetary bakery, the diversity of asteroids car) he fully appreciated, for to paraphrase Tolstoy, accreted planets are all alike; every unaccreted Planet is unaccreted in its own way.
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页码:413 / 448
页数:36
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