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Title:
Global stratigraphy of Venus: Analysis of a random sample of thirty-six test areas
Authors:
Basilevsky, Alexander T.; Head, James W., III
Affiliation:
AA(Brown University, Providence, RI, US), AB(Brown University, Providence, RI, US)
Publication:
Earth, Moon, and Planets (ISSN 0167-9295), vol. 66, no. 3, p. 285-336 (EM&P; Homepage)
Publication Date:
00/1995
Category:
Astronomy
Origin:
STI
NASA/STI Keywords:
Geochronology, Random Sampling, Stratigraphy, Structural Properties (Geology), Terrain, Venus (Planet), Cratering, Geomorphology, Magellan Spacecraft (Nasa), Mapping, Synthetic Aperture Radar, Volcanology
Bibliographic Code:
1995EM&P...66..285B

Abstract

The age relations between 36 impact craters with dark paraboloids and other geologic units and structures at these localities have been studied through photogeologic analysis of Magellan SAR images of the surface of Venus. Geologic settings in all 36 sites, about 1000 x 1000 km each, could be characterized using only 10 different terrain units and six types of structures. Mapping of such units and structures in 36 randomly distributed large regions shows evidence for a distinctive regional and global stratigraphic and geologic sequence. On the basis of this sequence we have developed a model that illustrates several major themes in the history of Venus. Most of the history of Venus (that of its first 80% or so) is not preserved in the surface geomorphological record. The major deformation associated with tessera formation in the period sometime between 0.5-1.0 b.y. ago (Ivanov and Basilevsky, 1993) is the earliest event detected. Our stratigraphic analyses suggest that following tessera formation, extensive volcanic flooding resurfaced at least 85% of the planet in the form of the presently-ridged and fractured plains. Several lines of evidence favor a high flux in the post-tessera period but we have no independent evidence for the absolute duration of ridged plains emplacement. During this time, the net state of stress in the lithosphere apparently changed from extensional to compressional, first in the form of extensive ridge belt development, followed by the formation of extensive wrinkle ridges on the flow units. Subsequently, there occurred local emplacement of smooth and lobate plains units which are presently essentially undeformed. The major events in the latest 10% of the presently preserved history of Venus are continued rifting and some associated volcanism, and the redistribution of eolian material largely derived from impact crater deposits. Detailed geologic mapping and stratigraphic synthesis are necessary to test this sequence and to address many of the outstanding problems raised by this analysis.

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