Planetary Atmospheres
Cover Page/Proposal Summary
ROSS-00 NRA 00-OSS-01
Date Due: 4/28/2000
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This proposal shall be used and disclosed for evaluation purposes only, and a copy of this Government notice shall be applied to any reproduction or abstract thereof. Any authorized restrictive notices that the submitter places on this proposal shall also be strictly complied with. Disclosure of this proposal for any reason outside the Government evaluation purposes shall be made only to the extent authorized by the Government. |
| Proposal Type: New Proposal |
| Proposal Category: Laboratory |
| Major Equipment Proposal? No |
| Do you intend to submit an Education/Public Outreach (E/PO) proposal? No |
| Proposal Title: |
| Chemical Weathering Reactions on Venus |
| Abbreviated Proposal Title: |
| Chemical Weathering Reactions on Venus |
| Principal Investigator: |
| Dr. Bruce Fegley Jr. Department of Earth & Planetary Sci. Washington University One Brookings Dr. Campus Box 1169 St. Louis, MO 63130-4899 Phone: 314-935-4852 Fax: 314-935-7361 E-mail: bfegley@levee.wustl.edu |
| Signature | Date |
| _____________________________________ | ____________ |
| Co-Investigators and Collaborators: | |||
| Type | Name | Affiliation | |
| Sci Collab | Dr. Goestar Klingelhoefer | Johannes Gutenberg Universitat | |
| Proposal Summary: | |
| We propose to continue using various experimental techniques and theoretical models to study chemical weathering reactions important for the present (and past) atmosphere-lithosphere cycles of volatiles (except sulfur, which is considered separately), and for the oxidation state of the present (and past) surface and atmosphere. These experiments and calculations are important for interpreting results from past space missions to Venus (Pioneer Venus, Magellan, Galileo flyby, Venera, and Vega), for interpreting results from Earth-based telescopic observations, and for the design of new (e.g., Discovery class) missions to Venus. Emphasis will be placed on two projects: (1) Hydrous silicate formation, stability, and decomposition, which is important for understanding the present and past atmosphere-lithosphere cycle for water on Venus and (2) Oxidation of Fe2+-bearing rock to Fe3+-bearing rock by atmospheric gases such as CO2 and H2O, which is important for understanding the redox state of the surface and atmosphere at present and oxygen loss and hydrogen escape to space over time. | |
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Willful provision of false information in this proposal and/or its supporting documents, or in reports required under an ensuing award, is a criminal offense (U.S. Code, Title 18, Section 1001). |



