Follow this link to go to the text only version of nasa.gov
NASA -National Aeronautics and Space Administration
Follow this link to skip to the main content
+ Text Only Site
+ Site Help & Preferences
Go
ABOUT NASALATEST NEWSMULTIMEDIAMISSIONSMyNASAWORK FOR NASA

+ Home
CASSINI-HUYGENS MISSION TO SATURN
CASSINI-HUYGENS MAIN
MULTIMEDIA
WHY CASSINI?
SPACECRAFT AND INSTRUMENTS
TIMELINE
CASSINI-HUYGENS TEAM
MEDIA RESOURCES
 + View Images
+ NASA Home > Mission Sections > Cassini-Huygens > Why Cassini?
Print ThisPrint This
Email ThisEmail This

FEATURES
Cassini Flyby: A Double Moon Saga

08.28.07

artist concept of Titan flyby Image right: Artist concept of Titan flyby. Image credit: NASA/JPL

Cassini flies near Titan on Aug. 31, 2007, gaining an opportunity to image the Huygens probe landing site and study the composition and geology of Titan's surface. This flyby also places Cassini on a course to conduct the closest flyby of the odd moon Iapetus that it will perform during the entire mission. On Sept. 10, Cassini will come about 1,640 kilometers (1,000 miles) from Iapetus' surface.

Iapetus is a world of sharp contrasts. The leading hemisphere is as dark as a freshly-tarred street, and the white, trailing hemisphere resembles freshly-fallen snow. Scientists want to know more about the composition of the dark material that coats Iapetus. They also want to learn more about Iapetus' distinctive walnut shape and the chain of mountains along its equator.

+ Back to Top



+ Freedom of Information Act
+ Budgets, Strategic Plans and Accountability Reports
+ The President's Management Agenda
+ Privacy Policy and Important Notices
+ Inspector General Hotline
+ Equal Employment Opportunity Data Posted Pursuant to the No Fear Act
+ Information-Dissemination Priorities and Inventories
+ USA.gov
+ ExpectMore.gov
NASA
Editor: Susan Watanabe
NASA Official: Brian Dunbar
Last Updated: August 28, 2007
+ Contact NASA
+ SiteMap