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On the left, Saturn's moon Enceladus is backlit by the sun, showing the fountain-like sources of the fine spray of material that towers over the south polar region. On the right, is a composite image of Titan. Credit: NASA/JPL/SSI and NASA/JPL/University of Arizona |
NASA's Cassini spacecraft is whipping through a double-header at Saturn to catch an up-close glimpse of two of the ringed planet's moons ? the icy geyser-ridden Enceladus and the cloud-covered Titan.
The fortuitous alignment of the two Saturn moons means that the Cassini probe will be able to observe these contrasting worlds within less than 48 hours, with no maneuver in between.
Cassini has already swooped by Enceladus, making its closest approach early on May 18 GMT (late at night on May 17 Pacific Time). The spacecraft passed within about 270 miles (435 km) of the moon's surface.
The main goal of the Enceladus flyby was to watch the sun behind the moon's water-rich plume that flares out from its south polar region.
Scientists used Cassini's ultraviolet imaging spectrograph to measure whether there is molecular nitrogen in the plume, which is already known to contain ammonia. Heat can allow ammonia molecules to break into nitrogen molecules and scientists want to know if that's happening at Enceladus.
By determining the nitrogen content of Enceladus' geyser plume, scientists could unearth clues about thermal processing in the interior of the icy moon.
Cassini's second flyby is taking it past Saturn's largest moon, Titan.
The closest approach will take place in the early hours of May 20 GMT, or late evening on May 19 Pacific time at NASA's Jet Propulsion Laboratory in Pasadena, Calif., where engineers watch over Cassini. The spacecraft will glide to within 750 miles (1,400 km) of the surface of the moon.
Cassini will perform radio science experiments as it passes Titan, in order to detect the subtle variations in the gravitational tug on the spacecraft by the giant moon, which is 25 percent larger in volume than the planet Mercury.
Scientists will analyze the data to get a clearer understanding of Titan's internal structure, and to learn whether the moon has a liquid ocean beneath its surface. The composite infrared spectrometer will also use its southernmost pass to collect thermal data to fill out its temperature map of the smoggy moon.
Cassini has made four previous flybys, with one more planned for the years ahead.
The Cassini probe launched in 1997 and arrived at Saturn in 2004, where it dropped the European Huygens probe on the cloudy surface of Titan. Cassini was slated to be decommissioned in September of this year, but has received an extended mission that now runs through 2017.
- Images - The Rings and Moons of Saturn
- Cassini's Latest Discoveries
- Special Report: Cassini's Mission to Saturn
