CONTROL OF THE BASEMENT STRUCTURE ON THE MORPHOLOGY OF OLYMPUS MONS VOLCANO (MARS)

被引：0

作者：

CIPA, A ^{[1
]}

BEBIEN, J ^{[1
]}

BONIN, B ^{[1
]}

BROUSSE, R ^{[1
]}

MASSON, P ^{[1
]}

机构：

[1] UNIV PARIS 11,GEOL DYNAM TERRE & PLANETES LAB,F-91405 ORSAY,FRANCE

来源：

COMPTES RENDUS DE L ACADEMIE DES SCIENCES SERIE II | 1992年 / 315卷 / 07期

关键词：

D O I：

暂无

中图分类号：

O [数理科学和化学]; P [天文学、地球科学]; Q [生物科学]; N [自然科学总论];

学科分类号：

07 ; 0710 ; 09 ;

摘要：

Olympus Mons volcano, on Mars, shows numerous structures trending NW-SE, NE-SW or N-S (basal scarp, terrace boundaries on the upper flanks, alignment of the craters making up the caldera...), parallel to structures observed around the volcano on Tharsis dome, This implies reactivation of old basement fractures during subsidence caused by the build up of the volcano.

引用

页码：801 / 806

页数：6

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