Cassini flyby of Saturn moon Enceladus offers insight into solar system history

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NASA’s Cassini spacecraft flew within 16 miles of Saturn’s moon Enceladus Oct. 9 to measure molecules in its space environment that could give insight into the history of the solar system.

This artist’s concept of Cassini shows the craft during the Saturn Orbit Insertion maneuver, just after the main engine has begun firing. The spacecraft is moving out of the plane and to the right (firing to reduce its spacecraft velocity with respect to Saturn) and has just crossed the ring plane. (Image by NASA/JPL) Below, this sweeping mosaic of Saturn’s moon Enceladus provides broad regional context for the ultra-sharp, close-up views NASA’s Cassini spacecraft acquired, during its flyby on Aug. 11. (Image by NASA/JPL/Space Science Institute)

“This encounter will potentially have far-reaching implications for understanding how the solar system was formed and how it evolved,” says professor Tamas Gombosi, chair of the Department of Atmospheric, Oceanic and Space Sciences.

Gombosi is the interdisciplinary scientist for magnetosphere and plasma science on the Cassini mission. His role is to coordinate studies that involve multiple plasma instruments on the spacecraft.

Enceladus is Saturn’s sixth-largest moon, orbiting within the planet’s outermost ring. It is approximately 313 miles in diameter.

In this flyby, Cassini was close enough to Enceladus to identify individual molecules in the moon’s space environment, including ions and isotopes. An ion is a charged particle, or a version of an element that has lost or gained negatively charged electrons. An isotope is a version of an element that has in its nucleus the typical protons for that element, but a different number of neutrons, thus exhibiting a different atomic weight.

The atoms around Enceladus are expected to hold clues to the past because they come from interior regions that have changed little since the moon was formed. Geysers near the moon’s south pole spew water and other molecules from the satellite’s interior. Because of Enceladus’ weak gravity and low atmospheric pressure, the water and gas molecules waft off to space.

The encounter will contribute to scientists’ understanding of how particles become charged and energized in Saturn’s magnetosphere. Also, when Cassini identifies the different isotopes in the space around the moon, it will help scientists discern the temperatures at various stages in Enceladus’ formation eons ago.

Cassini discovered the geysers on Enceladus in 2005. Scientists believe that there could be a liquid ocean beneath the moon’s surface. They also detected organic molecules at the moon in March. Organic molecules have carbon-hydrogen bonds, and are found in living organisms, and in comets.

“The mission as a whole is expected to bring central pieces of the solar system evolution puzzle into place,” says Gombosi, who also is the Rollin M. Gerstacker Professor of Engineering and a professor in the Department of Aerospace Engineering. “This encounter is expected to provide some of those puzzle pieces.”

This flyby marked Cassini’s fifth encounter with Enceladus. A sixth encounter, during which it will approach within 122 miles of the moon, is scheduled for Oct. 31. Four more flybys are planned in the next two years of Cassini’s extended mission, the Cassini Equinox Mission.

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