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Heat Pipe PlanetsWhen volcanism dominates heat transport, a terrestrial body enters a heat-pipe mode, in which hot magma moves through the lithosphere in narrow channels. Even at high heat flow, a heat-pipe planet develops a thick, cold, downwards-advecting lithosphere dominated by (ultra-)mafic flows and contractional deformation at the surface. Heat-pipes are an important feature of terrestrial planets at high heat flow, as illustrated by Io. Evidence for their operation early in Earth's history suggests that all terrestrial bodies should experience an episode of heat-pipe cooling early in their histories.
Document ID
20140012797
Acquisition Source
Johnson Space Center
Document Type
Conference Paper
Authors
Moore, William B.
(Hampton Univ. VA, United States)
Simon, Justin I.
(NASA Johnson Space Center Houston, TX, United States)
Webb, A. Alexander G.
(Louisiana State Univ. Baton Rouge, LA, United States)
Date Acquired
October 2, 2014
Publication Date
March 17, 2014
Subject Category
Lunar And Planetary Science And Exploration
Geophysics
Report/Patent Number
JSC-CN-30406
Report Number: JSC-CN-30406
Meeting Information
Meeting: Lunar and Planetary Science Conference
Location: The Woodlands, TX
Country: United States
Start Date: March 17, 2014
End Date: March 21, 2014
Sponsors: NASA Johnson Space Center, Universities Space Research Association, Lunar and Planetary Inst.
Distribution Limits
Public
Copyright
Public Use Permitted.
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