- Abstract:
-
Irregular mare patches (IMPs) are small volcanic features on the lunar nearside with young model ages. Several formation mechanisms have been proposed including: caldera collapse, explosive outgassing, lava flow inflation, pyroclastic eruption, and regolith drainage. We present new observations of the four largest IMPs (Sosigenes, In a, Cauchy-5, and Maskelyne) using the Lunar Reconnaissance Orbiter (LRO) Diviner Lunar Radiometer (Diviner) and evaluate the formation hypotheses in the context ...
Expand abstract - Publication status:
- Published
- Peer review status:
- Peer reviewed
- Publisher copy:
- 10.1016/j.icarus.2017.03.004
-
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- Publisher:
- Elsevier Publisher's website
- Journal:
- Icarus Journal website
- Volume:
- 290
- Pages:
- 224-237
- Publication date:
- 2017-03-09
- Acceptance date:
- 2017-03-08
- DOI:
- EISSN:
-
1090-2643
- ISSN:
-
0019-1035
- Pubs id:
-
pubs:689495
- URN:
-
uri:07865109-6d19-49d3-b787-4844cfbb39e2
- UUID:
-
uuid:07865109-6d19-49d3-b787-4844cfbb39e2
- Local pid:
- pubs:689495
- Keywords:
- Copyright date:
- 2017
Journal article
Young lunar volcanic features: Thermophysical properties and formation
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National Aeronautics and Space Administration
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