Detection of daily clouds on Titan

Caitlin Griffith, J. L. Hall, T. R. Gebelle

Research output: Contribution to journalArticle

112 Citations (Scopus)

Abstract

We have discovered frequent variations in the near-infrared spectrum of Titan, Saturn's largest moon, which are indicative of the daily presence of sparse clouds covering less than 1% of the area of the satellite. The thermodynamics of Titan's atmosphere and the clouds' altitudes suggest that convection governs their evolutions. Their short lives point to the presence of rain. We propose that Titan's atmosphere resembles Earth's, with clouds, rain, and an active weather cycle, driven by latent heat release from the primary condensible species.

Original languageEnglish (US)
Pages (from-to)509-513
Number of pages5
JournalScience
Volume290
Issue number5491
DOIs
StatePublished - 2000
Externally publishedYes

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Saturn
Rain
Atmosphere
Convection
Weather
Thermodynamics
Hot Temperature

ASJC Scopus subject areas

  • General

Cite this

Detection of daily clouds on Titan. / Griffith, Caitlin; Hall, J. L.; Gebelle, T. R.

In: Science, Vol. 290, No. 5491, 2000, p. 509-513.

Research output: Contribution to journalArticle

Griffith, C, Hall, JL & Gebelle, TR 2000, 'Detection of daily clouds on Titan', Science, vol. 290, no. 5491, pp. 509-513. https://doi.org/10.1126/science.290.5491.509
Griffith, Caitlin ; Hall, J. L. ; Gebelle, T. R. / Detection of daily clouds on Titan. In: Science. 2000 ; Vol. 290, No. 5491. pp. 509-513.
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