In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 124, No. 2 ( 2019-02), p. 418-436
Kurzfassung:
We computed the crystallization sequence of the lunar magma ocean to simulate the overturn of ilmenite‐bearing cumulates Stagnant lid formation prevents the overturn unless the reference viscosity at 1600 K is 10 20 Pa s or lower Independent of the rheological parameters, ilmenite cumulates sink as small‐scale diapirs
Materialart:
Online-Ressource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1029/2018JE005739
Sprache:
Englisch
Verlag:
American Geophysical Union (AGU)
Publikationsdatum:
2019
ZDB Id:
1086497-0
ZDB Id:
3094268-8
ZDB Id:
2016810-X
SSG:
16,13