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Updated: Jul 15, 2026

Simulation of the Planetary Interior Differentiation Processes in the Laboratory
06:04

Simulation of the Planetary Interior Differentiation Processes in the Laboratory

Published on: November 15, 2013

初期の火星の堆積岩は,初期の火星の堆積岩だった

M C Malin1, K S Edgett

  • 1Malin Space Science Systems, Post Office Box 910148, San Diego, CA 92191-0148, USA.

Science (New York, N.Y.)
|December 9, 2000
PubMed
まとめ

厚さ4キロメートルまでの巨大な火星の岩層は,ダイナミックな初期の堆積物の堆積を示しています. 湿気と乾燥の両方のプロセスがそれらの形成に寄与した可能性があり,複雑な地質学的歴史を示しています.

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Scattering And Absorption of Light in Planetary Regoliths11:34

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