Amplitude of heat flow variations on Mars from possible shoreline topography

Physics – Geophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

3

History Of Geophysics: Planetology, Planetology: Solar System Objects: Mars, Planetary Sciences: Heat Flow

Scientific paper

Analyses of the effective elastic thickness of the Martian lithosphere have been previously used to calculate surface heat flow on Mars at different places and times. In this work, I use elevation differences in a putative Late Hesperian shoreline, named Deuteronilus shoreline, and the relation between thermal state and buoyancy of the lithosphere, in order to estimate the amplitude of the variations of surface heat flow on Mars, probably related to the time in which this feature was formed. The results suggest that, if the Deuteronilus shoreline is a true paleo-equipotential surface, the relative amplitude of surface heat flow variations on the shoreline regions in the Late Hesperian were less than present-day ones in terrestrial continental areas. The results are also roughly valid for the outer contact of the Late Hesperian Vastitas Borealis Formation, if this contact is related to the limits of an ancient ocean. These results could imply that large areas of the Martian lithosphere have been tectonothermally stable since at least that time.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Amplitude of heat flow variations on Mars from possible shoreline topography 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 Amplitude of heat flow variations on Mars from possible shoreline topography, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Amplitude of heat flow variations on Mars from possible shoreline topography will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-1091328

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.