:,湿?

S W Squyres1, J F Kasting

  • 1Center for Radiophysics and Space Research, Cornell University, Ithaca, NY 14853, USA.

Science (New York, N.Y.)
|August 5, 1994
PubMed
概括

早期的火星可能由于地热和冲击而存在液态水,而不仅仅是降水. 温室气体 (如甲) 的温和变暖可能支了地表水流.

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