Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries

Details Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries

Mar 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001lpi....32.1329p&link_type=abstract

32nd Annual Lunar and Planetary Science Conference, March 12-16, 2001, Houston, Texas, abstract no.1329

Computer Science

Scientific paper

Magmatic differentiation of the Moon creates an incompatible
element-rich, dense residual mantle layer. To explain hemispheric
crustal asymmetries, we examine conditions for diapirically instablity
of this layer at spherical harmonic degree one.

Affiliated with

Also associated with

No associations

Rating

Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries 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 Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Gravitational Differentiation of an Initially Unstable Chemical Stratification: Origin of Lunar Asymmetries will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1615983