| タイトル | Titan Surface Temperatures from Cassini CIRS |
| 著者（英） | Nixon, C.A.; Carlson, R.C.; Romani, P.N.; Guandique, E.; Mamoutkine, A.A.; Bjoraker, M.H.; Albright, S.A.; Achterberg, R.K.; Bezard, B.; Coustenis, A.; Pearl, J.C.; Tingley, J.S.; Elliott, M.H.; Segura, M.E.; Samuelson, R.E.; Jennings, Donald E.; Kundle, V.G.; Brasunas, J.C.; Calcutt, S.; Courtin, R.; Flasar, F.M. |
| 著者所属（英） | NASA Goddard Space Flight Center |
| 発行日 | 2008-10-09 |
| 言語 | eng |
| 内容記述 | Thermal radiation from the surface of Titan reaches space through a spectral window at 19-microns wavelength. After removing the effects of the atmosphere, measurement of this radiance gives the brightness temperature of the surface. The Composite Infrared Spectrometer (CIRS) has made such measurements during the Cassini prime mission. These observations cover a wide range of emission angles, thereby constraining the contributions from atmospheric radiance and opacity. With the more complete latitude coverage and much larger dataset, we have been able to improve upon the original results from Voyager IRIS. CIRS measures an equatorial surface brightness temperature, averaged over longitude, of 93.7 +/- 0.6 K. This agrees with the HASI temperature at the Huygens landing site. The latitude dependence of surface brightness temperature exhibits an approximately 2 K decrease toward the South Pole and 3 K decrease toward the North Pole. The lower surface temperatures seen at high latitudes are consistent with conditions expected for lake formation. |
| NASA分類 | Lunar and Planetary Science and Exploration |
| 権利 | Copyright |
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