火星の観測史とは - わかりやすく解説 Weblio辞書

ウィキペディア

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火星の観測史

出典: フリー百科事典『ウィキペディア（Wikipedia）』 (2022/02/28 04:07 UTC 版)

火星の観測史(かせいのかんそくし)とは、火星観測の歴史である。本項目では紀元前2千年紀の古代エジプト天文学から遡って火星の観測史を説明する。

脚注

注釈

^ 中国でも紀元前69年に月による火星の掩蔽が観測されている
^ 1由旬はSurya Siddhantaにおいて約8kmである。
^ 位相とは満ち欠けのようなもののこと。月については月相を参照。
^ 現在は火星の直径は地球の直径の約53%であることが分かっている。
^ この地形は後にSinus Meridiani_(英語版)と呼ばれ、火星の子午線を通っている。
^ 後にこれは錯視であると見なされた。

出典

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