File:Cracks or Cryovolcanoes? Surface Geology Creates Clouds on Titan as Observed by Gemini and Keck (gemini0512a).jpg

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Captions

Captions

Gemini near-infrared adaptive optics images of Titan showing mid-latitude clouds at three infrared wavelength ranges: K', H2(1-0) and Br (gamma) (1.95-2.3, 2.1239 and 2.1686 respectively).

Summary

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Description
English: Gemini near-infrared adaptive optics images of Titan showing mid-latitude clouds at three infrared wavelength ranges: K', H2(1-0) and Br (gamma) (1.95-2.3, 2.1239 and 2.1686 respectively). The K'-band images show the surface, H2 reveals tropospheric cloud features (down from about 5-10km) and Br probes the lower stratosphere and upper troposphere. The resolution on these images is about 0.06". Note that the best examples of mid-latitude clouds occur on April 8th and May 4th.
Date 20 October 2005 (upload date)
Source Cracks or Cryovolcanoes? Surface Geology Creates Clouds on Titan as Observed by Gemini and Keck
Author Gemini Observatory
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