Wednesday, January 24

The jet stream of Titan

This artist's impression shows the 'light curve' produced by a star passing behind Titan, Saturn's biggest moon. When such occultation events take place, the light from the star is blocked out. Because Titan has a thick atmosphere, the light does not 'turn off' straight away. Instead, it drops gradually as the blankets of atmosphere slide in front of the star, as the light-curve drawn here shows. The way the light drops tells astronomers about the atmosphere of Titan. The peak at the center of the light curve represents the bright flash occurring at the very middle of the occultation. This is due to the fact that Titan's atmosphere acts as a lens, making the light emitted by the star passing behind converge into a focal point and produce the flash. Credit: ESA. Image by C. Carreau


The jet stream of Titan from PhysOrg.com

A pair of rare celestial alignments that occurred in November 2003 helped an international team of astronomers investigate the far-off world of Titan. In particular, the alignments helped validate the atmospheric model used to design the entry trajectory for ESA's Huygens probe.[...]

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