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Measuring the infrared radiation in Saturn’s and Titan’s atmospheres will reveal what molecules are present, their temperatures and velocities. This data will help scientists understand the climate of Saturn and its biggest moon and how those bodies formed an estimated 5 billion years ago, according to Carlson, a faculty member in CUA’s physics department who works at NASA’s Goddard center. The Cassini spectrometer that measures Saturn’s infrared radiation is one of 12 scientific instruments on board the spacecraft, which was launched in 1997 as a joint venture of NASA and the European Space Agency. Carlson’s task includes cleaning up the Cassini infrared radiation data, which has been contaminated by electrical noise from the spacecraft. Fifty percent larger than Earth’s moon, Titan is the only moon in our solar system with a dense atmosphere. Of special interest to astrophysicists, it is the only large body in the solar system that, like the Earth, contains water ice, abundant carbon, a nitrogen-based atmosphere and liquid lakes (composed of hydrocarbons). The infrared spectrometer data that Carlson is deciphering will also be used to determine the thermal structure of Saturn’s rings and to determine ring material composition and particle size, among other facts. The atmospheres of Saturn and Titan were largely a mystery before Cassini began transmitting its data, according to NASA. “It’s intoxicating to work in this field, studying the unknown, learning more about how planets and the solar system formed and thinking about deeper questions such as why we are here,” says Carlson. MEDIA: For more information, contact Katie Lee or Mary McCarthy in Catholic University’s Office of Public Affairs at 202-319-5600. —30— Last Revised 22-Jul-09 04:38 PM.
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