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- W1991424027 abstract "The composition and structure of icy conglomerate comet nuclei formed by an accumulation process in the primordial solar nebula is examined. In addition to the constituents usually proposed more complex and reactive molecules are expected. A significant proportion of compounds stable only at low temperatures should occur also. The mixture of ices and meteoric matter would form an aggregate with a density of a few tenths of a gm per cm3. An H2O-ice nucleus is stable to radii of 10 km. For larger objects compression begins to occur at the center causing the structure of small comets and the outer regions of large comets to differ from that of the interior. Cometary meteor showers suggest that such differences do exist." @default.
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- W1991424027 date "1963-01-01" @default.
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- W1991424027 title "The origin and structure of icy cometary nuclei" @default.
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- W1991424027 doi "https://doi.org/10.1016/0019-1035(63)90068-x" @default.
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