期刊
SCIENCE
卷 288, 期 5467, 页码 836-839出版社
AMER ASSOC ADVANCEMENT SCIENCE
DOI: 10.1126/science.288.5467.836
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Radar observations of the main-belt, M-class asteroid 216 Kleopatra reveal a dumbbell-shaped object with overall dimensions of 217 kilometers by 94 kilometers by 81 kilometers (+/-25%). The asteroid's surface properties are consistent with a regolith having a metallic composition and a porosity comparable to that of Lunar soil. Kleopatra's shape is probably the outcome of an exotic sequence of collisional events, and much of its interior may have an unconsolidated rubble-pile structure.
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