Planetary Atmospheres
Cover Page/Proposal Summary
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: Atmosphere Structures and Particles |
Major Equipment Proposal? No |
Do you intend to submit an Education/Public Outreach (E/PO) proposal? No |
Proposal Title: |
Research in Planetary Atmospheres-Jupiter and Titan(Continuation of Grant NAG5-4589) |
Abbreviated Proposal Title: |
Jupiter and Titan Atmospheric Composition & Str. |
Principal Investigator: |
Dr. Sushil K. Atreya Dept. Atmos. Ocean. & Space Sciences University of Michigan Space Research Bldg. Ann Arbor, MI 48109-2143 Phone: 734-763-6234 Fax: 734-764-5137 E-mail: atreya@umich.edu |
Signature | Date |
_____________________________________ | ____________ |
Co-Investigators and Collaborators: | |||
Type | Name | Affiliation | |
Sci Collab | Dr. Therese Encrenaz | Obs. Paris-Meudon | therese.encrenaz@obspm.fr |
Sci Collab | Dr. Paul R. Mahaffy | GSFC | paul.r.mahaffy@gsfc.nasa.gov |
Sci Collab | Dr. Hasso B. Niemann | GSFC | hasso.b.niemann@gsfc.nasa.gov |
Sci Collab | Dr. Tobias C. Owen | Univ. Hawaii | owen@ifa.hawaii.edu |
Proposal Summary:
Continuation of grant NAG5-4589 is proposed. Under the current grant,
observations from Galileo, HST and ISO were analyzed and interpreted.
We determined that the condensible volatiles (H2O, H2S, NH3) were
unexpectedly depleted to depths well below their equilibrium condensa-
tion levels in Jupiter’s deep troposphere. We have suggested that this
behavior, as well as the lack of substantial clouds, is a direct
consequence of local meteorology in the 5 micron hotspot, the entry
site of the Galileo probe. From the supersolar ratios (to H) of the
heavy elements (C,N,S,Ar,Kr,Xe) we measured, it was concluded that the
planetesimals that formed the core of Jupiter must have been very cold
(<30 K). The protosolar D/H value was fixed from an in situ Jovian D/H
measurement. We found the global values of eddy mixing in the
atmospheres of Uranus and Saturn to be comparable to the equatorial
values measured by Voyager. Eddy mixing coefficient in the upper
tropospheres and lower stratospheres of Jupiter and Saturn were also
derived. We propose to continue the analysis of the Galileo probe mass
spectrometer (GPMS) data, and make further progress on a model of the
chemical evolution of Titan’s atmosphere. Our goal is to characterize
the composition and structure of these bodies as fully as possible. In
particular, we will determine the distributions of C2 - and the
heavier hydrocarbons in the 1-20 bar range, the molecular nitrogen
abundance, and the nitrogen isotopic ratio in Jupiter’s atmosphere, by
analyzing the GPMS data. We will also refine our analysis of the
Jovian water vapor data. We will develop the model of chemistry of
Titan’s atmosphere further. All observational results will be
interpreted with coupled condensation-chemistry models to be developed
or updated simultaneously. Supporting data will be obtained from other
missions, in particular ISO.
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).