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冥王星の多角形地形を説明する力強いコンベクション

A J Trowbridge1, H J Melosh1,2, J K Steckloff2

  • 1Department of Earth, Atmospheric, and Planetary Sciences, Purdue University, West Lafayette, Indiana 47907, USA.

Nature
|June 3, 2016
PubMed
まとめ

冥王星のスプートニク・プランウムには窒素 (N2) の氷の多角形がある. N2氷層内のコンベクション電流は,若い地質学的に活発な表面を示唆する最も可能性が高い原因です.

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