The Tharsis Montes, Mars: Comparison of Volcanic and Modified Landforms

dc.contributor.author	Zimbelman, James R.
dc.contributor.author	Edgett, Kenneth S.
dc.contributor.author	https://orcid.org/0000-0002-0420-8453
dc.coverage.spatial	Mars (Planet)
dc.date.accessioned	2020-06-04T22:10:55Z
dc.date.available	2020-06-04T22:10:55Z
dc.date.issued	1992
dc.identifier.uri	https://hdl.handle.net/20.500.11753/1563
dc.description.abstract	The three Tharsis Montes shield volcanos, Arsia Mons, Pavonis Mons, and Ascraeus Mons, have broad similarities that have been recognized since the Mariner 9 reconnaissance in 1972. Upon closer examination the volcanos are seen to have significant differences that are due to individual volcanic histories.	en
dc.format.extent	Pages 31-44
dc.format.mimetype	application/pdf
dc.language.iso	en	en
dc.publisher	Lunar and Planetary Institute	en
dc.relation.ispartof	Proceedings of Lunar and Planetary Science, volume 22
dc.relation.ispartofseries	LPI contribution ; no. 774
dc.subject	Mars (Planet)--Volcanoes	en
dc.subject	Tharsis Montes (Mars)	en
dc.title	The Tharsis Montes, Mars: Comparison of Volcanic and Modified Landforms	en
dc.type	Book chapter	en

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