Radar Evidence for Liquid Surfaces on Titan

Donald B. Campbell, Gregory J. Black, Lynn M. Carter, Steven J. Ostro

Research output: Contribution to journalArticlepeer-review

88 Scopus citations


Arecibo radar observations of Titan at 13-centimeter wavelength indicate that most of the echo power is in a diffusely scattered component but that a small specular component is present for about 75% of the subearth locations observed. These specutar echoes have properties consistent with those expected for areas of liquid hydrocarbons. Knowledge of the areal extent and depth of any deposits of liquid hydrocarbons could strongly constrain the history of Titan's atmosphere and surface.

Original languageEnglish (US)
Pages (from-to)431-434
Number of pages4
Issue number5644
StatePublished - Oct 17 2003
Externally publishedYes

ASJC Scopus subject areas

  • General


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