THE GEOMORPHOLOGY AND EVOLUTION OF HECATE-CHASMA, VENUS

Citation
Ve. Hamilton et Er. Stofan, THE GEOMORPHOLOGY AND EVOLUTION OF HECATE-CHASMA, VENUS, Icarus, 121(1), 1996, pp. 171-194
Citations number
55
Categorie Soggetti
Astronomy & Astrophysics
Journal title
IcarusACNP
ISSN journal
00191035
Volume
121
Issue
1
Year of publication
1996
Pages
171 - 194
Database
ISI
SICI code
0019-1035(1996)121:1<171:TGAEOH>2.0.ZU;2-E
Abstract
Hecate Chasma is a discontinuous trough and fracture system extending from Atla Regio through Asteria Regio. A detailed examination of Hecat e Chasma using Magellan image and altimetry data reveals morphologic f eatures such as normal faults (including graben), compressional ridges , a variety of volcanic edifices, and coronae, There is no evidence fo r a systematic age progression among coronae in chains, thus a single, stationary thermal anomaly underlying a moving lithosphere is an unli kely origin for the chains, A comparison of the observed features with two possible models of evolution, subduction/delamination or lithosph eric extension with limited rifting, shows some similarities between t he predicted morphologies of each model and Hecate Chasma, The dominan ce of features related to upwelling and extensional tectonism strongly favor an extensional origin for this zone. The corona chain may have been formed by upwellings related to Rayleigh-Taylor instabilities, si milar to those observed at terrestrial mid-ocean ridges, but in an env ironment of limited spreading. (C) 1996 Academic Press, Inc.