Countdown to Controlled Collision
|Titan descent by Huygens probe leaving Cassini storage, Christmas 2004. Image Credit: JPL/Space Science Institute|
At 1.25 billion kilometers (750 million miles) from Earth, after a 7-year journey through the Solar system, the Huygens probe is about to separate from the Cassini orbiter to enter a ballistic trajectory toward Titan, the largest and most mysterious moon of Saturn, in order to dive into its atmosphere on 14 January.
This will be the first man-made object to explore in-situ this unique environment, whose chemistry is assumed to be very similar to that of the early Earth just before life began, 3.8 billion years ago.
The Cassini-Huygens pair, a joint mission conducted by NASA, ESA and the Italian Space Agency (ASI), was launched into space on October 15, 1997. With the help of several gravity assist maneuvers during flybys of Venus, Earth and Jupiter, it took almost 7 years for the spacecraft to reach Saturn.
The Cassini orbiter, carrying Huygens on its flank, entered an orbit around Saturn on 1 July 2004, and began to investigate the ringed planet and its moons for a mission that will last at least four years.
The first distant flyby of Titan took place on July 2-3, 2004. It provided data on Titan’s atmosphere which were confirmed by the data obtained during the first close flyby on October 26, 2004 at an altitude of 1174 km. These data were used to validate the entry conditions of the Huygens probe.
|The haze of an atmospheric layer on Saturn’s moon, Titan. Credit: Voyager Project, JPL, NASA|
A second close flyby of Titan by Cassini-Huygens at an altitude of 1200 km is scheduled on December 13 and will provide additional data to further validate the entry conditions of the Huygens probe.
On December 17 the orbiter will be placed on a controlled collision course with Titan in order to release Huygens on the proper trajectory, and on December 21 (some dates and times are subject to minor adjustment for operational reasons, except the entry time on January 14 which is known to within an accuracy of under 2 minutes) all systems will be set up for separation and the Huygens timers will be set to wake the probe a few hours before its arrival at Titan.
The Huygens probe is due to separate on the morning of December 25 at about 05:08 CET (Central European Time, 11:08 EST in the Eastern US on the December 24). Since the Cassini orbiter will have to achieve precise pointing for the release, there will be no real-time telemetry available until it turns back its main antenna toward Earth and beams the recorded data of the release. It will take over an hour (67 min) for the signals to reach us on Earth. The final data confirming the separation will be available later on Christmas Day.
After release, Huygens will move away from Cassini at a speed of about 35 centimeters per second and, to keep on track, will spin on its axis, making about 7 revolutions a minute. Huygens will not communicate with Cassini for the whole period until after deployment of the main parachute following entry into Titan’s atmosphere. On December 28 Cassini will then maneuver off collision course to resume its mission and prepare itself to receive Huygens data, which it will record for later playback to Earth.
|True color and surface infrared images show features resembling clouds and a continental area about the size of Australia Image Credit: NASA/JPL|
Huygens will remain dormant until a few hours before its arrival at Titan on January 14. The entry into the atmosphere is set for 11:15 CET. Huygens is planned to complete its descent in about two hours and 15 minutes, beaming back its science data to the Cassini orbiter for replay to Earth later in the afternoon. If Huygens, which is designed as an atmospheric probe rather than a lander, survives touchdown on the surface, it could deliver up to 2 hours of bonus data before the link with Cassini is lost.
Direct radio signals from Huygens will reach Earth after 67 minutes of interplanetary travel at the speed of light. An experiment has been set up by radio scientists that will use an array of radio telescopes around the Pacific to attempt to detect a faint tone from Huygens. If successful, early detection is not expected before around 11:30 CET.
Related Web Pages
Saturn Edition, Astrobiology Magaz.
Saturn’s Rings in UV
Cassini Closes In on Saturn
Saturn– JPL Cassini Main Page
Lord of the Rings
Space Science Institute, Imaging Team Boulder, Colorado
Saturn: The Closest Pass
Where is Cassini Now?