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Titan's atmospheric temperatures, winds, and composition

Authors :
Flasar, F.M.
Achterberg, R.K.
Conrath, B.J.
Gierasch, P.J.
Kunde, V.G.
Nixon, C.A.
Bjoraker, G.L.
Jennings, D.E.
Romani, P.N.
Simon-Miller, A.A.
Bezard, B.
Coustenis, A.
Irwin, P.G.J.
Teanby, N.A.
Brasunas, J.
Pearl, J.C.
Segura, M.E.
Carlson, R.C.
Mamoutkine, A.
Schinder, P.J.
Barucci, A.
Courtin, R.
Fouchet, T.
Gautier, D.
Lellouch, E.
Marten, A.
Prange, R.
Vinatier, S.
Strobel, D.F.
Calcutt, S.B.
Read, P.L.
Taylor, F.W.
Bowles, N.
Samuelson, R.E.
Orton, G.S.
Spilker, L.J.
Owen, T.C.
Spencer, J.R.
Showalter, M.R.
Ferrari, C.
Abbas, M.M.
Raulin, F.
Edgington, S.
Ade, P.
Wishnow, E.H.
Source :
Science. May 13, 2005, Vol. 308 Issue 5724, p975, 4 p.
Publication Year :
2005

Abstract

Temperatures obtained from early Cassini infrared observations of Titan show a stratopause at an altitude of 310 kilometers (and 186 kelvin at 15°S). Stratospheric temperatures are coldest in the winter northern hemisphere, with zonal winds reaching 160 meters per second. The concentrations of several stratospheric organic compounds are enhanced at mid- and high northern latitudes, and the strong zonal winds may inhibit mixing between these latitudes and the rest of Titan. Above the south pole, temperatures in the stratosphere are 4 to 5 kelvin cooler than at the equator. The stratospheric mole fractions of methane and carbon monoxide are (1.6 ± 0.5) x [10.sup.-2] and (4.5 ± 1.5) x [10.sup.-5] respectively.<br />Unlike other moons in the solar system, Titan has a substantial atmosphere and offers an interesting comparison with Earth and the other planets. Its pressure at the surface is 1.5 [...]

Details

Language :
English
ISSN :
00368075
Volume :
308
Issue :
5724
Database :
Gale General OneFile
Journal :
Science
Publication Type :
Academic Journal
Accession number :
edsgcl.132801891