Author/Authors :
Formisano، نويسنده , , V. and DʹAversa، نويسنده , , E. and Bellucci، نويسنده , , G. and Baines، نويسنده , , K.H. and Bibring، نويسنده , , J.P. and Brown، نويسنده , , R.H. and Buratti، نويسنده , , B.J. and Capaccioni، نويسنده , , F. and Cerroni، نويسنده , , P. and Clark، نويسنده , , R.N. and Coradini، نويسنده , , A. and Cruikshank، نويسنده , , D.P. and Drossart، نويسنده , , P. and Jaumann، نويسنده , , R. and Langevin، نويسنده , , Y. and Matson، نويسنده , , D.L. and McCord، نويسنده , , T.B. and Mennella، نويسنده , , V. and Nelson، نويسنده , , R.M. and Nicholson، نويسنده , , P.D. and Sicardy، نويسنده , , B. and Sotin، نويسنده , , C. and Chamberlain، نويسنده , , M.C. and Hansen، نويسنده , , G. and Hibbits، نويسنده , , K. and Showalter، نويسنده , , M. and Filacchione، نويسنده , , G.، نويسنده ,
Abstract :
We report unusual and somewhat unexpected observations of the jovian satellite Io, showing strong methane absorption bands. These observations were made by the Cassini VIMS experiment during the Jupiter flyby of December/January 2000/2001. The explanation is straightforward: Entering or exiting from Jupiterʹs shadow during an eclipse, Io is illuminated by solar light which has transited the atmosphere of Jupiter. This light, therefore becomes imprinted with the spectral signature of Jupiterʹs upper atmosphere, which includes strong atmospheric methane absorption bands. Intercepting solar light refracted by the jovian atmosphere, Io essentially becomes a “mirror” for solar occultation events of Jupiter. The thickness of the layer where refracted solar light is observed is so large (more than 3000 km at Ioʹs orbit), that we can foresee a nearly continuous multi-year period of similar events at Saturn, utilizing the large and bright ring system. During Cassiniʹs 4-year nominal mission, this probing technique should reveal information of Saturnʹs atmosphere over a large range of southern latitudes and times.
