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Tectonic evolution of Eastern Ishtar Terra, VenusTectonic deformation is cited as the cause for the complex morphology and topography of Eastern Ishtar Terra. A number of models proposed to account for this deformation are reviewed, and their predictions for the geology of Fortuna Tessera are examined. The detailed geology, topography, and structural fabric of Eastern Ishtar are reviewed, and these observations are compared to the predictions of the existing models for the formation and evolution of Fortuna Tessera. On the basis of the analysis, a number of conclusions are drawn regarding the evolution of Eastern Ishtar Terra. These include the recognition of primary morphological and topographical patterns which allow Eastern Ishtar Terra to be divided into four major physiographic regions named Maxwell Montes, Eastern Fortuna Tessera, Central Fortuna Tessera, and Northern Fortuna Tessera. A model is suggested that accounts for the morphology and high topography of Eastern Ishtar Terra.
Document ID
19910038987
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
External Source(s)
Authors
Vorder Bruegge, R. W.
(Brown Univ. Providence, RI, United States)
Head, James W.
(Brown University Providence, RI, United States)
Date Acquired
August 15, 2013
Publication Date
December 1, 1990
Publication Information
Publication: Earth, Moon, and Planets
Volume: 50-51
ISSN: 0167-9295
Subject Category
Lunar And Planetary Exploration
Report/Patent Number
ISSN: 0167-9295
Accession Number
91A23610
Funding Number(s)
CONTRACT_GRANT: NGR-40-002-116
CONTRACT_GRANT: NAGW-713
Distribution Limits
Public
Copyright
Other

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