![]() ![]() |
Current models for Titan's
atmosphere and surface will soon be tested in detail. This
will happen in 2004 by the instruments on-board the NASA/ESA Cassini mission. It is
the result of a 10-year collaboration between NASA and the European
Space Agency. The two institutions decided in 1987 to dedicate to
Titan an entire space mission that was named
Cassini/Huygens. Giovanni Cassini discovered the gap in
Saturn's rings in 1676. And the Huygens
module will arrive on Titan, very nearly 350 years after Christiaan
Huygens discovered Titan in 1655! The target of the Cassini/Huygens mission is the system of
Saturn, with its 18 satellites and seven rings. The spacecraft is
composed of an orbiter (Cassini) that will stay in orbit
around Saturn from 2004 on and will return data for at least four
years. Its other purpose is to deliver into Titan's atmosphere the
descent module, Huygens, for a two and a half hour
descent. Cassini carries 12 instruments, among which are
spectrometers, radar and cameras, while Huygens has a mass of
319 kg, is 2.5 m across, with six experimental instruments on board
that will penetrate the atmosphere of Titan and
make precise measurements of its density, pressure and temperature in
the lower 170 km. The Cassini spacecraft was successfully launched at 4:53
a.m. on the morning of 15 October 1997 from the Kennedy Space Centre at Cape
Canaveral (Florida). This mission is an extraordinary achievement of
scientific and technological breakthroughs resulting from a fruitful
collaboration between the US and 17 European countries. The launch was a great success. A roar marked the ignition and a
huge flame burnt the ground around the spacecraft, as it launched
towards the sky. At a height of about 16 km, the rocket boosters were
ejected, and the spacecraft, crossed the night sky like a bright comet
, starting on its seven-year course towards Saturn. The measurements
showed that the launch, as well as the adopted course, was performed
with great accuracy and according to schedule. The rocket, used for
the launch of the Cassini mission, had coincidentally the name
"Titan IV/Centaur". So Cassini was set on its way to Titan
by... Titan! Cassini is now well advanced on its course to Saturn (you may check
where it is now),
with planned arrival in July 2004. The Cassini orbiter has already returned data about Venus, Jupiter
and the Earth, when the spacecraft passed by these planets en
route. Everything is functioning well. Cassini will provide ten times more information than the Voyager
missions. Voyager data are still being analysed, today, 20 years
after the encounter, by many current and future astronomers. Can you
then imagine how long it will take to fully reduce and interpret the
large amounts of Cassini images and spectra? It is safe to predict that scientists of the coming generations will
be busy with them, well into the 22nd century.
|
![]()
Life in the Universe
Exploring the Solar System
Space Missions to the Outer Planets and their Moons
Titan - Saturn's Largest Moon
Titan's Atmosphere and Surface
The Cassini/Huygens Mission
![]()
Last updated August 1, 2001