In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 122, No. 12 ( 2017-12), p. 2510-2543
Kurzfassung:
Because of ongoing aeolian activity, the Bagnold dunes consist of well‐sorted sands and lack the finer grains typical of Martian soils Dune sands are chemically distinct with elevated Si, Mg, and Ni and lower H 2 O, S, and Cl relative to all previously measured Martian fines Two distinct, water‐/OH‐bearing amorphous components are identified: Fe‐, S‐, and Cl‐rich material in dust and Si‐rich material in the sands
Materialart:
Online-Ressource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1002/jgre.v122.12
DOI:
10.1002/2017JE005267
Sprache:
Englisch
Verlag:
American Geophysical Union (AGU)
Publikationsdatum:
2017
ZDB Id:
1086497-0
ZDB Id:
3094268-8
ZDB Id:
2016810-X
SSG:
16,13
