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ABSTRACT SINCE the detection by Pioneer 10 of an ionosphere1 around Io, this moon of Jupiter has been known to possess a tenuous atmosphere. The local observation of gaseous SO2 and the
upper limits on the concentrations of other gases deduced from Voyager data2, together with the identification of SO2 frost or adsorbate at the surface3,4 and upper limits on the global
amount of atmospheric SO2 (refs 5–8), have led to several classes of models for Io's atmosphere9. Here we report the microwave detection of SO2 at 222 GHz, which constitutes the first
direct global observation of Io's neutral atmosphere. The observations imply an SO2 surface pressure of 4–35 nanobars, covering 3–15% of the surface on both leading and trailing sides
of Io when illuminated by the Sun. This supports atmospheric models in which the partial pressure of SO2 at the surface is determined by the local surface temperature8, favouring, in
particular, the 'albedo cold-trap' models10,11. Our failure to detect H2S at 169 GHz suggests that the pressure of this gas is probably below 10 −10 bar. Our results, taken
together with the Pioneer ionospheric data, suggest that an atmospheric gas other than SO2 is present. We propose that the locally buffered SO2 atmosphere coexists with a background
atmosphere of oxygen with a partial surface pressure of ∼20 nanobars. Access through your institution Buy or subscribe This is a preview of subscription content, access via your institution
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about institutional subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS A SUBLIMATED WATER ATMOSPHERE ON GANYMEDE DETECTED FROM HUBBLE SPACE
TELESCOPE OBSERVATIONS Article 26 July 2021 LABORATORY PREDICTIONS FOR THE NIGHT-SIDE SURFACE ICE GLOW OF EUROPA Article 09 November 2020 DETECTION OF CARBON DIOXIDE AND HYDROGEN PEROXIDE ON
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1147–1151 (1972). Article ADS Google Scholar Download references AUTHOR INFORMATION AUTHORS AND AFFILIATIONS * Observatoire de Paris, 92195, Meudon, France Emmanuel Lellouch &
Thérèse Encrenaz * National Optical Astronomy Observatories, Tucson, Arizona, 85726, USA Michael Belton * Radio-Astronomy Department, University of California, Berkeley, California, 94720,
USA Imke de Pater * Jet Propulsion Laboratory, Pasadena, California, 91109, USA Samuel Gulkis Authors * Emmanuel Lellouch View author publications You can also search for this author
inPubMed Google Scholar * Michael Belton View author publications You can also search for this author inPubMed Google Scholar * Imke de Pater View author publications You can also search for
this author inPubMed Google Scholar * Samuel Gulkis View author publications You can also search for this author inPubMed Google Scholar * Thérèse Encrenaz View author publications You can
also search for this author inPubMed Google Scholar RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Lellouch, E., Belton, M., de Pater, I. _et al._
Io's atmosphere from microwave detection of SO2. _Nature_ 346, 639–641 (1990). https://doi.org/10.1038/346639a0 Download citation * Received: 12 April 1990 * Accepted: 27 June 1990 *
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