Exploration of the giant planets by infrared spectroscopyThe infrared spectrometer and radiometer for the Mariner-Jupiter-Saturn mission is described. Results of Nimbus and Mariner 9 IR spectroscopy of earth and Mars are used as examples to demonstrate the power and diversity of the technique. Determinations of planetary surface compositions, surface temperatures, vertical temperature profiles, surface pressures, and atmospheric constituents are summarized. Applications to Jupiter and Saturn are briefly mentioned.
Document ID
19770043815
Acquisition Source
Legacy CDMS
Document Type
Other - Collected Works
Authors
Hanel, R. A. (NASA Goddard Space Flight Center Laboratory for Atmospheric and Biological Sciences, Greenbelt, Md., United States)