Scientific Colloquium
February 24, 2006


Saturn’s largest moon, Titan, remains an enigma, explored only by remote sensing from Earth, and by the Voyager and Cassini spacecraft. The most puzzling aspects include the origin of the molecular nitrogen and methane in its atmosphere, and the mechanisms by which methane is maintained in the face of rapid destruction by photolysis. The Huygens probe, launched from the Cassini spacecraft, has made the first direct observations of the lower atmosphere and the moon’s surface. The Huygens probe carried six experiments to measure atmospheric structure, winds, chemical composition and optical properties of the atmosphere and the aerosols, and surface properties. The probe reached the upper atmosphere of Titan on January 14, 2005, and landed softly on the surface after a 2.5 hour descent. Unexpectedly, it transmitted data from the surface for 69 minutes giving additional clues about the surface composition and morphology.