Geographic control of Titan's mid-latitude clouds

Henry G. Roe, Michael E. Brown, Emily L. Schaller, Antonin H. Bouchez, Chadwick A. Trujillo

Research output: Contribution to journalArticlepeer-review

75 Scopus citations


Observations of Titan's mid-latitude clouds from the W. M. Keck and Gemini Observatories show that they cluster near 350°W longitude, 40°S latitude. These clouds cannot be explained by a seasonal shift in global circulation and thus presumably reflect a mechanism on Titan such as geysering or cryovolcanism in this region. The rate of volatile release necessary to trigger cloud formation could easily supply enough methane to balance the loss to photolysis in the upper atmosphere.

Original languageEnglish (US)
Pages (from-to)477-479
Number of pages3
Issue number5747
StatePublished - Oct 21 2005
Externally publishedYes

ASJC Scopus subject areas

  • General


Dive into the research topics of 'Geographic control of Titan's mid-latitude clouds'. Together they form a unique fingerprint.

Cite this