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Geologic map of part of the Tyrrhena Patera region of Mars (MTM Quadrangle-20252)

IMAP 2556
By: , and 

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Abstract

Mars Transverse Mercator (MTM) -20252 quadrangle contains the volcano Tyrrhena Patera, a low, broad structure that has summit depressions and is dissected by prominent radial channels (fig. 1). Tyrrhena Patera is surrounded by cratered plains materials on the western edge of Hesperia Planum, ~2,000 km northeast of the center of the Hellas basin (Greeley and Guest, 1987; U. S. Geological Survey, 1991). On the basis of Mariner 9 data, Tyrrhena Patera was interpreted to be a shield volcano, composed of fluid basic or ultrabasic lavas (Peterson, 1978; Pike, 1978). Analysis of Viking Orbiter images led Greeley and Spudis (1981) to suggest that Tyrrhena Patera comprises pyroclastic deposits produced by explosive hydromagmatic eruption; Greeley and Crown (1990) support a pyroclastic origin for Tyrrhena Patera shield materials and assess several eruption styles for the volcano (see also Crown and Greeley, 1993).

Publication type Report
Publication Subtype USGS Numbered Series
Title Geologic map of part of the Tyrrhena Patera region of Mars (MTM Quadrangle-20252)
Series title IMAP
Series number 2556
ISBN 0607917830
DOI 10.3133/i2556
Year Published 1998
Language English
Publisher U.S. Geological Survey
Description 1 Plate: 65.40 × 54.75 inches
Other Geospatial Mars, Tyrrhena Patera
Scale 502000
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Additional publication details