In situ measurements of the physical characteristics of Titan's environment

• Published in: Nature Vol. 438; no. 7069; pp. 785 - 791
• Main Authors: López-Moreno, J. J, Flamini, E, Harri, A. M, Coustenis, A, Seiff, A, Trautner, R, Fulchignoni, M, Mäkinen, T, Towner, M. C, McDonnell, J. A. M, Fanti, G, Lion Stoppato, P. F, Debei, S, Barucci, M. A, Schwingenschuh, K, Borucki, W, Zarnecki, J. C, Bianchini, G, Colombatti, G, Molina-Cuberos, G, Falkner, P, Bar-Nun, A, Lehto, A, Leese, M. R, Angrilli, F, McKay, C. P, Tokano, T, Ferri, F, Saggin, B, Hathi, B, Grard, R, Jernej, I, Bettanini, C, Rodrigo, R, Gaborit, V, Coradini, M, Simões, F, Ball, A. J, Neubauer, F. M, Pirronello, V, Withers, P, Svedhem, H, Hamelin, M
• Format: Journal Article
• Language: English
• Published: England Nature Publishing Group 08.12.2005
• Subjects: Astrophysics; Atmospheric electricity; Atmospheric pressure; Cosmology and Extra-Galactic Astrophysics; In situ measurement; Lightning; Methane; Moons; Nitrogen; Physics; Plasma Physics; Sciences of the Universe; Temperature
• ISSN: 0028-0836; 1476-4687; 1476-4679
• DOI: 10.1038/nature04314

On the basis of previous ground-based and fly-by information, we knew that Titan's atmosphere was mainly nitrogen, with some methane, but its temperature and pressure profiles were poorly constrained because of uncertainties in the detailed composition. The extent of atmospheric electricity ('lightning') was also hitherto unknown. Here we report the temperature and density profiles, as determined by the Huygens Atmospheric Structure Instrument (HASI), from an altitude of 1,400 km down to the surface. In the upper part of the atmosphere, the temperature and density were both higher than expected. There is a lower ionospheric layer between 140 km and 40 km, with electrical conductivity peaking near 60 km. We may also have seen the signature of lightning. At the surface, the temperature was 93.65 +/- 0.25 K, and the pressure was 1,467 +/- 1 hPa.