When the Huygens probe descends through Titan’s atmosphere on January 14, only one optical instrument will be available for imaging. The Descent Imager/Spectral Radiometer (DISR) will take photographs of the surface during the two-hour descent, relaying the data to the Cassini orbiter for re-transmission to the Deep Space Network. Martin Tomasko of the University of Arizona’s Lunar and Planetary Laboratory leads the international team in charge of DISR; he and other UA colleagues will head for the European Space Operations Center in Darmstadt, Germany next week.
Key points:
The first data should arrive shortly after 2 PM EST on Friday January 14. Images should be available by the early morning of the 15th. A news conference will be held the same morning at ESOC to present initial results.
We are now seven days away from the most distant landfall ever attempted.
Sources: University of Arizona Lunar and Planetary Laboratory press release; Jet Propulsion Laboratory. Also, check the Cassini VIMS Science Investigations site for information about the Visual and Infrared Mapping Spectrometer aboard the orbiter.