,

Joshua L Bandfield1

  • 1School of Earth and Space Exploration, Arizona State University, Tempe, Arizona 85287-6305, USA. joshband@asu.edu

Nature
|May 4, 2007
PubMed
まとめ

水氷は火星の浅い地表で安定しており,その深さは緯度によって異なります. 新しい熱画像は局所的な変化を明らかにし,活発な火星の水循環と氷床の深さに影響を与える要因を示唆しています.

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