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遠地点

5 件の記事

The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1)

アプシス(近点・遠点)とは天体軌道の極点とそのメカニズム

アプシス近点遠点軌道要素
The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1)

近点と遠点(アプシス)天体軌道の極値とそのメカニズム

アプシス近点遠点近日点
The apsides refer to the farthest (2) and nearest (3) points reached by an orbiting planetary body (2 and 3) with respect to a primary, or host, body (1)

近点と遠点(アプシス)天体軌道の極値とそのメカニズム

アプシス近点遠点近日点
Variation of the distance between the centers of the Moon and the Earth over 700 days

月と地球の距離変動する軌道と測定の歴史

地球平均距離近地点
Orbital dynamics of the Moon, with exaggerated paths and sizes, particularly illustrating that the Moon's orbit is on average slightly more outbound than inbound around the Sun, perturbed by Earth.[6]

月軌道のメカニズム地球とのダイナミックな相互作用

軌道地球重心