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: Tenuous Atmospheres |
| Major Equipment Proposal? No |
| Do you intend to submit an Education/Public Outreach (E/PO) proposal? No |
| Proposal Title: |
| Effects of Radiation on Desorption of Alkalis from Mineral and Ice Surfaces: Relation to Origins of Alkali Vapor in Planetary Atmospheres |
| Abbreviated Proposal Title: |
| Desorption of Alkali Atoms from Minerals and Ices |
| Principal Investigator: |
| Dr. Theodore Madey Physics and Astronomy Rutgers University 136 Frelinghuysen Rd. Piscataway, NJ 08854-8019 Phone: 732-445-5185 Fax: 732-445-4991 E-mail: madey@physics.rutgers.edu |
| Signature | Date |
| _____________________________________ | ____________ |
| Co-Investigators and Collaborators: | |||
| Type | Name | Affiliation | |
| Sci Collab | Prof. Vladimir Ageev | A. F. Ioffe Physico-Technical Institute, Russia | ageev@ms.ioffe.rssi.ru |
| Sci Collab | Prof. Robert E. Johnson | Univ. of Virginia | rej@virginia.edu |
| Sci Co-I | Dr. Boris V. Yakshinskiy | Rutgers University | yaksh@physics.edu |
| Proposal Summary: | |
| We propose to use laboratory methods to address the origins of alkali vapors (Na, K) in the atmospheres of the planet Mercury, the Moon, and Europa. We will use a variety of ultrahigh-vacuum surface science techniques to make measurements of thermal desorption and radiation-induced desorption (i.e., by electrons, photons, and ions) of Na and K from the surfaces of model minerals characteristic of planetary and lunar surfaces, and from ice surfaces characteristic of Europa. We will build on our recent studies of desorption of Na from SiO_{2} surfaces, where we have shown that photon-stimulated desorption is a probable major source process for Na in the lunar atmosphere. Substrates will include amorphous and crystalline H_{2}O ice surfaces, amorphous and crystalline Al_{2}O_{3}, and amorphous SiO_{2}. We will also study more complex mineral substrates (olivine or plagioclase) as closer surrogates for the lunar and Mercurian surfaces; we will apply to NASA for lunar samples. Adsorption (sticking) probabilities, desorption yields, energy thresholds and kinetic energy distributions will be determined for both Na and K, and the effect of substrate electronic properties (e.g., bandgap) will be determined. We will test a one-electron charge-transfer model of photon stimulated desorption, which may provide insights into why Na and K (but not Mg and Ca) are seen in the atmospheres. We expect that these data will provide useful input to modelers and theorists who are simulating tenuous planetary atmospheres. | |
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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). |



