01-070 |
ROSS-00 NRA 00-OSS-01
Date Due: 4/28/2000
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: |
Origins of the Atmospheres of Mercury and the Moon |
Abbreviated Proposal Title: |
Origins of the atmospheres of Mercury and the Moon |
Principal Investigator: |
Dr. Rosemary M. Killen Instrumentation and Space Research Division 15 Southwest Research Institute 6220 Culebra Road P.O. Drawer 28510 San Antonio, TX 78228-0510 Phone: 210-522-2719 Fax: 210-543-0052 E-mail: rosemary@whipple.space.swri.edu |
Signature | Date |
_____________________________________ | ____________ |
Co-Investigators and Collaborators: | |||
Type | Name | Affiliation | |
Sci Co-I | Dr. Andrew E. Potter Jr. | LPI | potter@lpi.jsc.nasa.gov |
Sci Collab | Dr. Patricia Reiff | Rice Univ. | reiff@alfven.rice.edu |
Sci Collab | Dr. Bernard Jackson | UCSD | BJackson@cass01.ucsd.edu |
Sci Collab | Dr. Barbara Giles | Goddard SFC | bgiles@lepvax.gsfc.nasa.gov |
Proposal Summary:
The planet Mercury is subject to the same space-weather related phenomena that occur at Earth - but on a much shorter timescale since the spatial scales involved are smaller, the magnetic field is weaker, and the solar wind flux is approximately an order of magnitude larger. While the analogy is imperfect, there is great advantage to study of a system which is far enough away that the entire atmosphere can be imaged at once, and which responds to changes in the interplanetary environment on timescales of a few minutes. We have already shown that the exosphere responds to changes in the magnetosphere in response to the changing solar wind pressure and the IMF. The details of this interaction are still relatively uncertain. However, in addition to the alkali species, we now have observations of an additional species, Ca, which appears to be promoted into the atmosphere by ion sputtering. This hypothesis is controversial, and rightly so, since our data set is limited. We will pose and answer the following specific questions 1) how does the solar cycle affect the exosphere of Mercury, 2) and what does this tell us about the relative roles of meteoritic vaporization, photon-stimulated desorption and ion sputtering as source processes? Can observations of Mercury's exosphere at eastern elongation be used statistically to predict space weather at Earth approximately six days later? We will reduce and publish 13 years of observations of the Hermean atmosphere, compute the column abundance, model the source rates for the three proposed source processes, and compare observations with predictions of the model. Our colleagues at UCSD will provide solar wind density and speed at Mercury. Our colleagues at Rice University will provide us with magnetosphere models required to accurately model the ion sputter source for the atmosphere of Mercury.
Certification of Compliance with Applicable Executive Orders and U.S. Code
By submitting the proposal identified in this Cover Sheet/Proposal Summary in response to this NRA or AO, the Authorizing Official of the proposing institution (or the individual proposer if there is no proposing institution) as identified below:
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).