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Do Titan's Mountains Betray the Late Acquisition of its Current AtmosphereTitan may have acquired its massive atmosphere relatively recently in solar system history [1,2,3,4]. Prior to that time, Titan would have been nearly airless, with its volatiles frozen or sequestered. Present-day Titan experiences only small (approximately 4 K) pole-to-equator variations, owing to efficient heat transport via the thick atmosphere [5]; these temperature variations would have been much larger (approximately 20 K) in the absence of an atmosphere. If Titan's ice shell is conductive, the change in surface temperature associated with the development of an atmosphere would have led to changes in shell thickness. In particular, the poles would move down (inducing compression) while the equator would move up. Figure 1 shows the predicted change in surface elevation as a result of the change in surface temperature, using the numerical conductive shell thickness model of [6]
Document ID
20120013423
Acquisition Source
Ames Research Center
Document Type
Conference Paper
Authors
Moore, Jeffrey Morgan
(NASA Ames Research Center Moffett Field, CA, United States)
Nimmo, F.
(California Univ. Santa Cruz, CA, United States)
Date Acquired
August 26, 2013
Publication Date
October 2, 2011
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN3978
Meeting Information
Meeting: EPSC-DPS Joint Meeting 2011
Location: Nantes
Country: France
Start Date: October 2, 2011
End Date: October 7, 2011
Funding Number(s)
WBS: WBS 202844.02.02.01.89
Distribution Limits
Public
Copyright
Public Use Permitted.
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