NEW $CO_{2}$ BANDS IN THE CONNES' VENUS SPECTRA.
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Date
1966
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Ohio State University
Abstract
Venus spectra in the $1.3 \mu, 1.6 \mu$ and $2 \mu$ regions have recently been obtained by P. and J. Connes using a Michelson interferometer. Many new bands of carbon dioxide are identified in these spectra, some of which have never been observed in the laboratory spectra due to lack of either sufficiently long path lengths of absorbing gas or high enough resolution. Preliminary estimates of the relative abundance of $(O^{17}/O^{16}), (O^{18}/O^{16})$ and $(C^{13}/C^{12})$ are presented for Venus.
Description
Author Institution: Space Science Division, Jet Propulsion Laboratory