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The role of regolith adsorption in the transition from early to late Mars climateResearchers reexamined radiative transfer models of early Mars that were advanced to show the existance of a greenhouse effect. These models were reexamined with regard to the effect that regolith adsorption may have had. It is argued that while the precipitation of carbonates has probably been an important process during Mars history, the rates at which this process could have taken place under early Mars conditions would have dropped sharply once liquid water was fairly scarce. Furthermore, conditions under which liquid water was available may have involved efficient recycling of carbonate so that steady state conditions rather than irreversible CO2 removal prevailed. In contrast, the growth of regolith surface area demands corresponding and predictable CO2 removal from the atmosphere-cap system and is fully capable of terminating any enhanced temperature regime on early Mars in the absence of any other effects.
Document ID
19870013978
Acquisition Source
Legacy CDMS
Document Type
Other
Authors
Fanale, F. P.
(Hawaii Univ. Honolulu, HI, United States)
Postawko, S. E.
(Hawaii Univ. Honolulu, HI, United States)
Zent, A. P.
(Hawaii Univ. Honolulu, HI, United States)
Salvail, J. R.
(Hawaii Univ. Honolulu, HI, United States)
Date Acquired
September 5, 2013
Publication Date
May 1, 1987
Publication Information
Publication: NASA, Washington, Reports of Planetary Geology and Geophysics Program, 1986
Subject Category
Lunar And Planetary Exploration
Accession Number
87N23411
Distribution Limits
Public
Copyright
Work of the US Gov. Public Use Permitted.
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