In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 123, No. 4 ( 2018-04), p. 823-848
Abstract:
With 1‐D thermal evolution models in Monte Carlo simulations we find north/south crustal properties that fit Mars's elastic thickness estimates Our results suggest that 55–65% of the bulk radioelement content are in the crust, mostly in the southern one (43–51%) We retrieve a north/south surface heat flux of 17.1–19.5 mW/m 2 and 24.8–26.5 mW/m 2 , respectively, that could influence InSight measurements
Type of Medium:
Online Resource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1002/2017JE005431
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2018
detail.hit.zdb_id:
1086497-0
detail.hit.zdb_id:
3094268-8
detail.hit.zdb_id:
2016810-X
SSG:
16,13
