Follow this link to skip to                                      the main content

Feature

Text Size

Cassini-Huygens Top 10 Science Highlights
07.20.05
 
After nearly seven years of space travel, the Cassini-Huygens mission arrived at Saturn in July 2004. The mission's first year has returned intriguing science results and stunning images of the ringed world and its varied moons. And this is just the beginning.
  1. The Cassini Orbiter and the Huygens Probe Reveal Titan's Earth-Like Surface and Organic Atmosphere.
  2. Closest-Ever Observations of Saturn's Rings Reveal Clumps, Kinks, Moons and Waves.
  3. Phoebe: A Captured World From the Outer Solar System
  4. Saturn's Dynamic Atmosphere
  5. Enceladus: A Moon With a Tenuous Atmosphere
  6. Saturn's New Radiation Belt
  7. Ever-Changing Ring-Moon Interactions
  8. Saturn May Be Slowing Down
  9. Iapetus Equatorial Mountain Range
  10. Dione: A Moon With Wispy Terrain
Artist concept depicting the Huygens probe departing the Cassini spacecraft near TitanImage right: Artist's concept of Huygens probe as it is released from Cassini spacecraft. Huygens is headed towards Saturn's moon Titan. Image credit: NASA/JPL.

A year after entering orbit around Saturn, the Cassini-Huygens team is looking back at a string of remarkable discoveries. Numerous discoveries have been made about Titan's surface and atmosphere, Saturn's magnificent rings, its amazing moons, dynamic magnetosphere and the planet itself. The highlight of the mission so far is clearly the lifting of the veil on smog-covered Titan. The orbiter's remarkable instruments provided the first glimpses of the surface and the global picture of the hazy world. The Huygens probe touchdown provided a close-up look of a whole new world, much like our own.

What scientists expected to see and did not see is equally interesting. The scientists' original ideas for Titan's surface included global oceans and lakes of liquid hydrocarbons. The Huygens probe was even designed to float briefly, since a liquid landing was deemed very likely. Small lakes may exist, but global oceans are just not there. This lack of large bodies of liquid may cause scientists to rethink the age and origin of Titan's atmosphere.

Spokes in Saturn's B ring, as seen by NASA's Voyager spacecraft, were also anticipated. To date, we have not seen spokes in geometries where they should have been seen if their associated dust clouds were present. This lack of spokes shows that important electrostatic or electrodynamic effects, like photoelectric charging of the rings, vary seasonally.

On July 14, Cassini made its closest flyby yet, swinging about 175 kilometers (109 miles) above the surface of Saturn's moon Enceladus. Other exciting events include flybys of "six worlds in 80 days," including two flybys of Titan and one each of the moons Tethys, Hyperion, Dione and Rhea. During the October flyby of Titan we will obtain a radar swath over the Huygens landing site, which will help scientists put the rest of Titan in context with the portion studied in detail by the probe.


+ Part II - Discoveries

 
 
Carolina Martinez (818) 354-9382
Jet Propulsion Laboratory, Pasadena, Calif.