Author/Authors :
Cavalié، نويسنده , , T. and Billebaud، نويسنده , , F. and Dobrijevic، نويسنده , , M. and Fouchet، نويسنده , , T. and Lellouch، نويسنده , , E. and Encrenaz، نويسنده , , T. and Brillet، نويسنده , , J. and Moriarty-Schieven، نويسنده , , G.H. and Wouterloot، نويسنده , , J.G.A. and Hartogh، نويسنده , , P.، نويسنده ,
Abstract :
We have performed the first observation of the CO(3-2) spectral line in the atmosphere of Saturn with the James Clerk Maxwell Telescope. We have used a transport model of the atmosphere of Saturn to constrain the origin of the observed CO. The CO line is best-fit when the CO is located at pressures less than ( 15 ± 2 ) mbar with a mixing ratio of ( 2.5 ± 0.6 ) × 10 - 8 implying an external origin. By modeling the transport in Saturn’s atmosphere, we find that a cometary impact origin with an impact 200–350 years ago is more likely than continuous deposition by interplanetary dust particles (IDP) or local sources (rings/satellites). This result would confirm that comet impacts are relatively frequent and efficient providers of CO to the atmospheres of the outer planets. However, a diffuse and/or local source cannot be rejected, because we did not account for photochemistry of oxygen compounds. Finally, we have derived an upper limit of ∼ 1 × 10 - 9 on the tropospheric CO mixing ratio.
