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The Tethered MoonCosmic collisions between terrestrial planets resemble somewhat the life cycle of the phoenix: worlds collide, are consumed in flame, and after the debris has cleared, shiny new worlds emerge aglow with possibilities. And glow they do, for they are molten. How brightly they glow, and for how long, is determined by their atmospheres and their moons. A reasonable initial condition on Earth after the Moon-forming impact is that it begins as a hot global magma ocean. We therefore begin our study with the mantle as a liquid ocean with a surface temperature on the order of 3000-4000 K at a time some 100-1000 years after the impact, by which point we can hope that early transients have settled down.
Document ID
20140013201
Acquisition Source
Ames Research Center
Document Type
Reprint (Version printed in journal)
Authors
Zahnle, K.
(NASA Ames Research Center Moffett Field, CA United States)
Lupu, R.
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Dobrovolskis, A.
(Search for Extraterrestrial Intelligence Inst. Moffett Field, CA, United States)
Date Acquired
October 24, 2014
Publication Date
March 17, 2014
Subject Category
Lunar And Planetary Science And Exploration
Report/Patent Number
ARC-E-DAA-TN12989
Report Number: ARC-E-DAA-TN12989
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: Lunar and Planetary Inst., Universities Space Research Association, NASA Johnson Space Center
Funding Number(s)
CONTRACT_GRANT: NNX13AD56A
WBS: WBS 132379.04.05.09
CONTRACT_GRANT: NNX12AJ19A
Distribution Limits
Public
Copyright
Public Use Permitted.
Keywords
the existence of the Moon
terrestrial planets
substantial atmosphere
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