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・ Vallikkunnu
・ Vallikunnam
・ Vallila
・ Vallimalai
・ Vallin
・ Vallinam
・ Vallinfreda
・ Vallini
・ Vallio Terme
・ Vallipuram
・ Vallipuram Vasanthan
・ Valliquerville
・ Vallirana
・ Vallis
・ Vallis (planetary geology)
Vallis Alpes
・ Vallis Baade
・ Vallis Bohr
・ Vallis Bouvard
・ Vallis Ex Umbra De Mortuus
・ Vallis Inghirami
・ Vallis Planck
・ Vallis Rheita
・ Vallis Schrödinger
・ Vallis Snellius
・ Vallis Vale
・ Valliscaulian Order
・ Vallisneria
・ Vallisneria americana
・ Vallisneria spiralis


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Vallis Alpes : ウィキペディア英語版
Vallis Alpes

Vallis Alpes (latin for"Alpine Valley") is a lunar valley feature that bisects the Montes Alpes range. It extends 166 km from the Mare Imbrium basin, trending east-northeast to the edge of the Mare Frigoris. The valley is narrow at both ends and widens to a maximum width of about 10 km along the middle stretch. The selenographic coordinates of this feature are .
The valley floor is a flat, lava-flooded surface that is bisected by a slender, cleft-like rille. (This cleft is a challenging target for telescope observation from the Earth.) The sides of the valley rise from the floor to the surrounding highland terrain, a blocky, irregular surface. The southern face of the valley is straighter than the northern side, which is slightly bowed and uneven. The more rugged edges of the valley lie at the narrow west-southwest end that cuts through the mountain range. Most likely this valley is a graben that was subsequently flooded with magma from Mare Imbrium and Mare Frigoris.
This valley was discovered in 1727 by Francesco Bianchini.
==References==


抄文引用元・出典: フリー百科事典『 ウィキペディア(Wikipedia)
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