Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth

Details Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth

Mar 2010

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2010lpi....41.2085o&link_type=abstract

41st Lunar and Planetary Science Conference, held March 1-5, 2010 in The Woodlands, Texas. LPI Contribution No. 1533, p.2085

Computer Science

Scientific paper

We compute Coulomb failure conditions to assess likely failure criteria
at Enceladus’s tiger stripes, exploring a suite of model
parameters (e.g. ice shell thickness, fault depth, frictional
coefficient) that inhibit or promote shear fault failure.

Affiliated with

Also associated with

No associations

Rating

Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth 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 Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Investigating the Limits of Enceladus's Tidally Driven Tiger Stripe Failure Scenario: Exploration of Ice Shell Thickness, Coefficient of Friction, and Fault Depth will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1207339