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Updated: Jul 12, 2026

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface
06:14

Simulating Imaging of Large Scale Radio Arrays on the Lunar Surface

Published on: July 30, 2020

月面のレゴリティは,静寂基地の静寂基地にあります

E M Shoemaker, M H Hait, G A Swann

    Science (New York, N.Y.)
    |January 30, 1970
    PubMed
    まとめ

    3~6メートルの厚さの瓦層であるTranquillity Baseのレゴライトは,その厚さと断片の露出をクレーター分布と結びつけるためにモデル化することができます. この月のレゴリットモデルは,表面の進化と衝撃の歴史を理解するのに役立ちます.

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