In:
Journal of Geophysical Research: Planets, American Geophysical Union (AGU), Vol. 129, No. 2 ( 2024-02)
Abstract:
Irregular mare patches appear to be dominated by high‐calcium pyroxene, are glass‐poor, and spectrally similar to their host mare and nearby fresh craters The lack of significant glass and similarity to their host mare do not strongly support a recent eruption of juvenile magmatic material, effusive or pyroclastic, or glassy foam exposed at the surface IMPs are likely composed of mare‐like materials that have been recently modified, such as through outgassing or regolith drainage into subsurface voids
Type of Medium:
Online Resource
ISSN:
2169-9097
,
2169-9100
DOI:
10.1029/2023JE008108
Language:
English
Publisher:
American Geophysical Union (AGU)
Publication Date:
2024
detail.hit.zdb_id:
1086497-0
detail.hit.zdb_id:
3094268-8
detail.hit.zdb_id:
2016810-X
SSG:
16,13
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