In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 122, No. 7 ( 2017-07), p. 1505-1521
Kurzfassung:
Volumes of mare basalts within five basins on the lunar farside are estimated The minimum crustal thicknesses within the basins were a dominant factor determining whether magma erupted at the surface Magma production on the farside was ~20 times smaller than that on the nearside
Materialart:
Online-Ressource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1002/2016JE005246
Sprache:
Englisch
Verlag:
American Geophysical Union (AGU)
Publikationsdatum:
2017
ZDB Id:
1086497-0
ZDB Id:
3094268-8
ZDB Id:
2016810-X
SSG:
16,13