Published 1998
| Published
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Shock wave equations of state of chondritic meteorites
- Creators
- Anderson, William W.
- Ahrens, Thomas J.
Chicago
Abstract
We have obtained shock compression data for Murchison and Bruderheim chondritic meteorites. Data for Murchison suggest that the Hugoniot states are described by a smooth curve to ≥90 GPa, having ρ_0=2.656 Mg/m^3, K_(S0)=24.2±.7 GPa, K′=4.17±.10, and constant γ=1.0. The data for Bruderheim suggest more complicated behavior. A mineral mixture model consistent with the Bruderheim data suggests that the Hugoniot state is a low pressure phase below 25 GPa, with ρ_0=3.555 Mg/m^3, K_(S0)=146 GPa, K′=2.53, and constant ργ=7.11 Mg/m^3; and a high pressure phase above 65 GPa, with ρ_0=4.40 Mg/m^3, K_(S0)=225 GPa, K′=3.25, and constant ργ=7.485 Mg/m^3.
Additional Information
© 1998 The American Institute of Physics. Published online 10 July 1998. We thank Prof. Dr. Dieter Stöffler of the Museum für Naturkunde, Berlin, for providing the samples and E. Gelle and M. Long for assistance with the experiments. Contribution #6213, Division of Geological and Planetary Sciences. California Institute of Technology. Research supported by NASA.Attached Files
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Additional details
- Eprint ID
- 50694
- Resolver ID
- CaltechAUTHORS:20141022-144202210
- NASA
- Created
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2014-10-23Created from EPrint's datestamp field
- Updated
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2021-11-10Created from EPrint's last_modified field
- Series Name
- AIP conference proceedings
- Series Volume or Issue Number
- 429
- Other Numbering System Name
- Caltech Division of Geological and Planetary Sciences
- Other Numbering System Identifier
- 6213