NASA Logo

NTRS

NTRS - NASA Technical Reports Server

Back to Results
Pioneer Venus gas chromatography of the lower atmosphere of VenusA gas chromatograph mounted in the Pioneer Venus sounder probe measured the chemical composition of the atmosphere of Venus at three altitudes. Ne, N2, O2, Ar, CO, H2O, SO2, and CO2 were measured, and upper limits set for H2, COS, H2S, CH4, Kr, N2O, C2H4, C2H6, and C3H8. Simulation studies have provided indirect evidence for sulfuric acid-like droplets and support the possibility of water vapor at altitudes of 42 and 24 km. The paper discusses the implications of these results for the origin, evolution, and present state of Venus' atmosphere.
Document ID
19810042400
Acquisition Source
Legacy CDMS
Document Type
Reprint (Version printed in journal)
Authors
Oyama, V. I.
(NASA Ames Research Center Moffett Field, CA, United States)
Carle, G. C.
(NASA Ames Research Center Moffett Field, CA, United States)
Woeller, F.
(NASA Ames Research Center Moffett Field, CA, United States)
Pollack, J. B.
(NASA Ames Research Center Moffett Field, CA, United States)
Reynolds, R. T.
(NASA Ames Research Center Moffett Field, CA, United States)
Craig, R. A.
(NASA Ames Research Center Moffett Field, Calif., United States)
Date Acquired
August 11, 2013
Publication Date
December 30, 1980
Publication Information
Publication: Journal of Geophysical Research
Volume: 85
Subject Category
Lunar And Planetary Exploration
Accession Number
81A26804
Distribution Limits
Public
Copyright
Other

Available Downloads

There are no available downloads for this record.
No Preview Available