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Science 1 July 1983: Vol. 221. no. 4605, pp. 55 - 57 DOI: 10.1126/science.221.4605.55
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Articles
Oceans on Titan?
F. M. FLASAR 1
1 Laboratory for Extraterrestrial Physics, NASA/Goddard Space Flight Center, Greenbelt, Maryland 20771
If global oceans of methane exist on Titan, the atmosphere above them must be within 2 percent of saturation. The two Voyager radio occultation soundings, made at low latitudes, probably occurred over land, since they imply a relative humidity 70 percent near the surface. Oceans might exist at other low-latitude locations if the zonal wind velocities in the lowest 3 kilometers are 4 centimeters per second.
Submitted on November 30, 1982
Revised on March 28, 1983
THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
- Storms, polar deposits and the methane cycle in Titan's atmosphere.
- C. A. Griffith (2009)
Phil Trans R Soc A
367, 713-728
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- Evidence for the Exposure of Water Ice on Titan's Surface.
- C. A. Griffith, T. Owen, T. R. Geballe, J. Rayner, and P. Rannou (2003)
Science
300, 628-630
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- Detection of Daily Clouds on Titan.
- C. A. Griffith, J. L. Hall, and T. R. Geballe (2000)
Science
290, 509-513
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- Radar Reflectivity of Titan.
- D. O. Muhleman, D. O. Muhleman, A. W. Grossman, B. J. Butler, and M. A. Slade (1990)
Science
248, 975-980
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- Probing Titan's Surface.
- V. R. Eshleman, V. R. ESHLEMAN, G. L. TYLER, R. A. SIMPSON, and E. A. MAROUF (1984)
Science
223, 772
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- Microwave Measurements of Carbon Monoxide on Titan.
- D. O. Muhleman, D. O. MUHLEMAN, G. L. BERGE, and R. T. CLANCY (1984)
Science
223, 393-396
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- Ethane Ocean on Titan.
- J. I. Lunine, J. I. LUNINE, D. J. STEVENSON, and Y. L. YUNG (1983)
Science
222, 1229-1230
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- Is Titan Wet or Dry?.
- V. R. Eshleman, V. R. ESHLEMAN, G. F. LINDAL, and G. L. TYLER (1983)
Science
221, 53-55
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