Note to users. If you're seeing this message, it means that your browser cannot find this page's style/presentation instructions -- or possibly that you are using a browser that does not support current Web standards. Find out more about why this message is appearing, and what you can do to make your experience of our site the best it can be.


Science 13 May 2005:
Vol. 308. no. 5724, pp. 975 - 978
DOI: 10.1126/science.1111150

Reports

Titan's Atmospheric Temperatures, Winds, and Composition

F. M. Flasar,1* R. K. Achterberg,2 B. J. Conrath,3 P. J. Gierasch,3 V. G. Kunde,4 C. A. Nixon,4 G. L. Bjoraker,1 D. E. Jennings,1 P. N. Romani,1 A. A. Simon-Miller,1 B. Bézard,5 A. Coustenis,5 P. G. J. Irwin,6 N. A. Teanby,6 J. Brasunas,1 J. C. Pearl,1 M. E. Segura,7 R. C. Carlson,2 A. Mamoutkine,2 P. J. Schinder,3 A. Barucci,5 R. Courtin,5 T. Fouchet,5 D. Gautier,5 E. Lellouch,5 A. Marten,5 R. Prangé,5 S. Vinatier,5 D. F. Strobel,8{dagger} S. B. Calcutt,6 P. L. Read,6 F. W. Taylor,6 N. Bowles,6 R. E. Samuelson,4 G. S. Orton,9 L. J. Spilker,9 T. C. Owen,10 J. R. Spencer,11 M. R. Showalter,12 C. Ferrari,13 M. M. Abbas,14 F. Raulin,15 S. Edgington,9 P. Ade,16 E. H. Wishnow17

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 10-2 and (4.5 ± 1.5) x 10-5, respectively.

1 NASA/Goddard Space Flight Center, Code 693, Greenbelt, MD 20771, USA.
2 Science Systems and Applications, 5900 Princess Garden Parkway, Suite 300, Lanham, MD 20706, USA.
3 Department of Astronomy, Cornell University, Ithaca, NY 14853, USA.
4 Department of Astronomy, University of Maryland, College Park, MD 20742, USA.
5 Laboratoire d'Études Spatiales et d'Instrumentation en Astrophysique (LESIA), CNRS–Unité Mixte de Recherche (UMR) 8109, Observatoire de Paris, 5 place Jules Janssen, F-91925 Meudon Cedex, France.
6 Atmospheric, Oceanic, and Planetary Physics, Clarendon Laboratory, Parks Road, University of Oxford, Oxford OX1 3PU, UK.
7 QSS Group, 4500 Forbes Boulevard, Suite 200, Lanham, MD 20706, USA.
8 Department of Earth and Planetary Science, Johns Hopkins University, Baltimore, MD 21218, USA.
9 Jet Propulsion Laboratory, 4800 Oak Grove Drive, Pasadena, CA 91109, USA.
10 University of Hawaii, Institute of Astronomy, 2680 Woodlawn Drive, Honolulu, HI 96822, USA.
11 Department of Space Studies, Southwest Research Institute, 1050 Walnut Street, Suite 400, Boulder, CO 80302, USA.
12 Search for Extraterrestrial Intelligence (SETI) Institute, 515 North Whisman Road, Mountain View, CA 94043, USA.
13 Commissariat de l'Énergie Atomique, Saclay, Service d'Astrophysique, 91191 Gif-sur-Yvette Cedex, France.
14 NASA/Marshall Space Flight Center, SD50 NSSTC, Huntsville, AL 35812, USA.
15 Laboratoire Interuniversitaire des Systèmes Atmosphériques, Université de Paris 7 and 12, CNRS-UMR 7583, 61 Avenue General de Gaulle, 94010 Creteil Cedex, France.
16 Department of Physics and Astronomy, University of Cardiff, 5 The Parade, Cardiff CF24 3YB, UK.
17 Lawrence Livermore National Laboratory and Space Sciences Laboratory, University of California, Berkeley, L-041, Livermore, CA 94551, USA.

{dagger} Present address: LESIA, CNRS-UMR 8109, Observatoire de Paris, 5 place Jules Janssen, F-91925 Meudon Cedex, France.

* To whom correspondence should be addressed. E-mail: f.m.flasar{at}nasa.gov

Read the Full Text



THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
The structure and dynamics of Titan's middle atmosphere.
F.M Flasar and R.K Achterberg (2009)
Phil Trans R Soc A 367, 649-664
   Abstract »    Full Text »    PDF »
The coupling of winds, aerosols and chemistry in Titan's atmosphere.
S. Lebonnois, P. Rannou, and F. Hourdin (2009)
Phil Trans R Soc A 367, 665-682
   Abstract »    Full Text »    PDF »
Dynamical implications of seasonal and spatial variations in Titan's stratospheric composition.
N. A Teanby, P. G.J Irwin, R. de Kok, and C. A Nixon (2009)
Phil Trans R Soc A 367, 697-711
   Abstract »    Full Text »    PDF »
Storms, polar deposits and the methane cycle in Titan's atmosphere.
C. A. Griffith (2009)
Phil Trans R Soc A 367, 713-728
   Abstract »    Full Text »    PDF »
Inaugural Article: Organic haze on Titan and the early Earth.
M. G. Trainer, A. A. Pavlov, H. L. DeWitt, J. L. Jimenez, C. P. McKay, O. B. Toon, and M. A. Tolbert (2006)
PNAS 103, 18035-18042
   Abstract »    Full Text »    PDF »
Evidence for a polar ethane cloud on Titan..
C. A. Griffith, P. Penteado, P. Rannou, R. Brown, V. Boudon, K. H. Baines, R. Clark, P. Drossart, B. Buratti, P. Nicholson, et al. (2006)
Science 313, 1620-1622
   Abstract »    Full Text »    PDF »
The Evolution of Titan's Mid-Latitude Clouds.
C. A. Griffith, P. Penteado, K. Baines, P. Drossart, J. Barnes, G. Bellucci, J. Bibring, R. Brown, B. Buratti, F. Capaccioni, et al. (2005)
Science 310, 474-477
   Abstract »    Full Text »    PDF »
Intensive Titan Exploration Begins.
P. R. Mahaffy (2005)
Science 308, 969-970
   Abstract »    Full Text »    PDF »
Ion Neutral Mass Spectrometer Results from the First Flyby of Titan.
J. H. Waite Jr., H. Niemann, R. V. Yelle, W. T. Kasprzak, T. E. Cravens, J. G. Luhmann, R. L. McNutt, W.-H. Ip, D. Gell, V. De La Haye, et al. (2005)
Science 308, 982-986
   Abstract »    Full Text »    PDF »



To Advertise     Find Products


Science. ISSN 0036-8075 (print), 1095-9203 (online)