Tectonic Modes and Atmospheric Argon on Venus and Earth

Details Tectonic Modes and Atmospheric Argon on Venus and Earth Tectonic Modes and Atmospheric Argon on Venus and Earth

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2177h&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2177

Physics

Scientific paper

Differences in tectonic histories of Venus and Earth result from
different convective stresses and can be understood with melting and
degassing models constrained by the atmospheric abundance of radiogenic
argon.

Affiliated with

Also associated with

No associations

Rating

Tectonic Modes and Atmospheric Argon on Venus and Earth does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Tectonic Modes and Atmospheric Argon on Venus and Earth, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Tectonic Modes and Atmospheric Argon on Venus and Earth will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1392431