A final trajectory correction maneuver is scheduled for June 16. On arrival date, June 30, Cassini will become the first spacecraft to orbit Saturn. Once in orbit it will conduct an extensive, four-year tour of the Saturn system, including its majestic rings and many known moons.
"The arrival date and trajectory to Saturn were specifically selected to accommodate this flyby, which will be the only opportunity during the mission to study Phoebe at close range," said Dave Seal, mission planner for the Cassini-Huygens mission at NASA's Jet Propulsion Laboratory, Pasadena, Calif. "Phoebe's orbit is simply too far from Saturn, at almost 13 million kilometers (about 8 million miles), nearly four times as far as the next closest major satellite, Iapetus. A later encounter is not feasible."
"The last time we had observations of Phoebe was by Voyager in 1981," said Dr. Torrence Johnson, former Voyager imaging team member, Galileo project scientist and current Cassini imaging team member. "This time around, the pictures of the mysterious moon will be about 1,000 times better, as Cassini will be closer." Voyager 2 captured images of Phoebe from about 2.2 million kilometers (about 1.4 million miles) away. Cassini will obtain images from a mere 2,000 kilometers (about 1,240 miles) above the moon's surface.
Cassini will also collect spectroscopic and radar data that could decipher the composition and origin of this distant moon. Cassini's Phoebe images, already twice as good as any image returned by Voyager 2, show large craters and variation in surface brightness.
"We anticipate that Phoebe will be heavily cratered in the higher resolution images we expect to see in the next few days," said Dr. Peter Thomas, a member of the imaging team and a senior research associate at Cornell University, Ithaca, N.Y., who specializes in studies of small satellites. "The hints of different brightnesses also suggest that the highest resolution images, several hundred times better, will show a variety of materials.
Discovered in 1898 by American astronomer William Henry Pickering, Phoebe is of great interest to scientists. "With the instruments Cassini carries, we might learn more about Phoebe's internal structure and composition. What we have are many unanswered questions: Did it ever melt? Does it have evidence of past interior melting? Was it ever an icy body? Why is Phoebe in such an odd orbit?" said Dr. Dennis Matson, project scientist for the Cassini-Huygens mission at JPL.
Phoebe has a diameter of 220 kilometers (about 136.7 miles), which is equal to about one-fifteenth the diameter of Earth's moon. Phoebe rotates on its axis every nine hours and 16 minutes, and it completes a full orbit around Saturn in about 18 months. Its elliptical orbit is inclined approximately 30 degrees to Saturn's equator. Phoebe's retrograde orbit means that it goes around Saturn in the opposite direction of the larger interior Saturnian moons. Previous ground-based observations have shown water ice present on its surface.
Phoebe is also unusual in that it is very dark. It reflects only six percent of the sunlight it receives. Phoebe's darkness and retrograde orbit suggest that it is most likely a captured object. A captured object is a celestial body that is caught by the gravitational pull of a much bigger body, generally a planet. Some scientists believe Phoebe might even be an object from the outer solar system, similar to the objects found in the Kuiper Belt. The Kuiper Belt is a collection of small icy bodies beyond Pluto that were never drawn together by gravity to form a planet.
"The dark and odd-shaped Phoebe may be a piece of the building blocks from which some of the planets formed," said Dr. Bonnie Buratti, scientist on the Cassini-Huygens mission at JPL. "It might hold clues about the early formation of our solar system."
The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. JPL designed, developed and assembled the Cassini orbiter.
For information about the Cassini-Huygens mission to Saturn and Titan on the Internet, visit: http://www.nasa.gov/cassini or http://www.esa.int/Cassini-Huygens.
For information about NASA and agency programs on the Internet, visit http://www.nasa.gov.
Carolina Martinez (818) 354-9382
Jet Propulsion Laboratory, Pasadena, Calif.
Dwayne Brown (202) 358-1726
NASA Headquarters, Washington, D.C.
2004-145