Cassini-Huygens Spacecraft

Cassini-Huygens is one of the most ambitious missions ever launched into space. Loaded with an array of powerful instruments and cameras, the spacecraft is capable of taking accurate measurements and detailed images in a variety of atmospheric conditions and light spectra.

Two elements comprise the spacecraft: The Cassini orbiter and the Huygens probe. In 2004, Cassini-Huygens is scheduled to reach Saturn and its moons. There the spacecraft will orbit around the system for four years; beaming home valuable data that will help us understand the vast Saturnian region. Huygens will enter the murky atmosphere of Titan, Saturn's biggest moon, and eventually descend via parachute onto its mysterious surface. The Huygens probe will send its measurements and images to Cassini, which will then beam them back to Earth.

Cassini-Huygens is a three-axis stabilized spacecraft equipped for 27 diverse science investigations. The Cassini orbiter has 12 instruments and the Huygens probe has six. The instruments often have multiple functions, equipped to thoroughly investigate all the important elements that the Saturn system may uncover. The spacecraft communicates through one high-gain and two-low gain antennas. It is only in the event of a power failure or other such emergency situation however, that the spacecraft will communicate through one of its low-gain antennas, known as LGA-1.

Three Radioisotope Thermoelectric Generators -- commonly referred to as RTGs -- provide power for the spacecraft, including the instruments, computers, and radio transmitters on board, attitude thrusters, and reaction wheels.

Cassini-Huygens Spacecraft with "almost human" features

In some ways, the Cassini spacecraft has senses better than our own. For example, Cassini can "see" in wavelengths of light and energy that the human eye cannot. The instruments on the spacecraft can "feel" things about magnetic fields and tiny dust particles that no human hand could detect.

The science instruments can be classified in a way that can be compared to the way human senses operate. Your eyes and ears are "remote sensing" devices because you can receive information from remote objects without being in direct contact with them. Your senses of touch and taste are "direct sensing" devices. Your nose can be construed as either a remote or direct sensing device. You can certainly smell the apple pie across the room without having your nose in direct contact with it, but the molecules carrying the scent do have to make direct contact with your sinuses. Cassini's instruments can be classified as remote and microwave remote sensing instruments, and fields and particles instruments--these are all designed to record significant data and take a variety of close-up measurements.

The remote sensing instruments on the Cassini Spacecraft can calculate measurements from a great distance. This set includes both optical and microwave sensing instruments including cameras, spectrometers, radar and radio.

The fields and particles instruments take "in situ" (on site) direct sensing measurements of the environment around the spacecraft. These instruments measure magnetic fields, mass, electrical charges and densities of atomic particles. They also measure the quantity and composition of dust particles, the strengths of plasma (electrically charged gas), and radio waves.