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Discovery of Temperate Latitude Clouds on Titan
Author(s) -
H. G. Roe,
Antonin H. Bouchez,
Chadwick A. Trujillo,
E. L. Schaller,
Michael E. Brown
Publication year - 2004
Publication title -
the astrophysical journal
Language(s) - English
Resource type - Journals
SCImago Journal Rank - 2.376
H-Index - 489
eISSN - 1538-4357
pISSN - 0004-637X
DOI - 10.1086/427499
Subject(s) - titan (rocket family) , latitude , troposphere , solstice , southern hemisphere , atmospheric sciences , insolation , climatology , physics , astrobiology , astronomy , geology
Until now, all the clouds imaged in Titan's troposphere have been found at far southern latitudes (60-90 south). The occurrence and location of these clouds is thought to be the result of convection driven by the maximum annual solar heating of Titan's surface, which occurs at summer solstice (2002 October) in this south polar region. We report the first observations of a new recurring type of tropospheric cloud feature, confined narrowly to ∼40 south latitude, which cannot be explained by this simple insolation hypothesis. We propose two classes of formation scenario, one linked to surface geography and the other to seasonally evolving circulation, which will be easily distinguished with continued observations over the next few years. Subject headings: infrared: solar system — planets and satellites: individual (Titan) Online material: color figure

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