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Title: Properties of Planetary Fluids at High Shock Pressures and Temperatures

Conference · · Geophysical Monograph (Online)
DOI:https://doi.org/10.1029/gm067p0387· OSTI ID:5947167
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  1. Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)

Models of the interiors of Uranus and Neptune are discussed. Pressures and temperatures in the interiors can be achieved in representative constituent molecular fluids by shock compression. Experimental techniques are described and recent results for synthetic Uranus and hydrogen are discussed.

Research Organization:
Lawrence Livermore National Laboratory (LLNL), Livermore, CA (United States)
Sponsoring Organization:
USDOE; National Aeronautics and Space Administration (NASA)
DOE Contract Number:
W-7405-ENG-48; W 16.180
OSTI ID:
5947167
Report Number(s):
UCRL-JC-106880; CONF-910196-1; ON: DE91011195; CNN: W16.180
Journal Information:
Geophysical Monograph (Online), Conference: 4. U.S. Japan Seminar on High Pressure Research in Mineral Physics: Applications to Earth and Planetary Sciences, Ise (Japan), 15-18 Jan 1991; ISSN 2328-8779
Publisher:
American Geophysical Union (AGU)
Country of Publication:
United States
Language:
English

References (17)

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