Water vapour in the atmosphere of a transiting extrasolar planet (2007)
Tinetti, G., Vidal-Madjar, A., Yung, Y., Carey, S., ...
Water is predicted to be among the most abundant (if not the most abundant) molecular species after hydrogen in the atmospheres of close-in extrasolar giant planets ('hot Jupiters'). Several attempts...
Boesch, Hartmut, Toon, G., Sen, B, Li, Q. B., Salawitch, R., Miller, C., ...
NASA/JPL
Boesch, Hartmut, Toon, G., Sen, B, Li, Q.B., Salawitch, R., Miller, C., ...
NASA/JPL
Infrared Transmission Spectra for Extrasolar Giant Planets (2006)
Tinetti, G., Liang, M. C., Vidal-Madjar, A., Ehrenreich, D., Etangs, A. Lecavelier Des, Yung, Y.
Among the hot Jupiters that transit their parent stars known to date, the two best candidates to be observed with transmission spectroscopy in the mid-infrared (MIR) are HD189733b and HD209458b, due...
Enceladus’ water vapour plumes (2006)
Hansen, Candice J., Esposito, L., Colwell, J., Hendrix, A., Matson, Dennis, Parkinson, C., ...
NASA/JPL
OH Column abundance over TMF 1997 - 2000 (2004)
Yung, Y., Mills, F., Sander, S., Cageao, R., Nemtchinov, V., Jiang, Y., ...
The column abundance of OH over the Jet Propulsion Laboratory's Table Mountain Facility (TMF) has been measured regularly since July 1997 using the Fouier-Transform Ultraviolet Spectrometer.
Evolution of the Martian Atmosphere: Results of a Monte Carlo Model of Sputtering (2004)
Using a Monte-Carlo model, we determine the sputtering yields for the upper atmosphere of Mars at three different epochs (the present, ~2.5 Gyr ago and ~3.5 Gyr ago).
CARBON DIOXIDE ON TITAN (1982)
Maguire, W. C., Hanel, R., Jennings, D., Kunde, V. G., Samuelson, R., Aikin, A., ...
$^{1}$R. Hanel. et. al., Science 212, 192 (1981). $^{2}$W.C. Maguire, et. al., Nature 292, 683 (1981). $^{3}$V.G. Kunde, et. al., Nature 292, 686 (1981).