Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism

Details Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism

Mar 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011lpi....42.2329f&link_type=abstract

42nd Lunar and Planetary Science Conference, held March 7–11, 2011 at The Woodlands, Texas. LPI Contribution No. 1608, p.2329

Physics

Scientific paper

A model of the subsurface thermal environment beneath Titan’s
Sotra Facula cryovolcanic construct is presented and implications for
ammonia-water cryovolcanism are discussed.

Affiliated with

Also associated with

No associations

Rating

Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism 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 Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Geological Processes on Titan Driven by Low Thermal Conductivity Volatile-Rich Deposits: Implications for Ammonia-Water Cryovolcanism will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1393421