Sunday, September 7th, 2008

Photo

<p>A Cassini spacecraft wide-angle camera view shows a half-lit
Saturn, with two dark storms rolling

A Cassini spacecraft wide-angle camera view shows a half-lit Saturn, with two dark storms rolling

UCLA scientists use spacecraft to explore formation of solar system

Cassini-Huygens orbits Saturn to study rings, magnetic field, Titan’s surface

A solitary spacecraft 750 miles away orbits Saturn, gathering information about the giant planet’s moons, rings, atmosphere and magnetic field that may help scientists recreate the formation of the solar system and the origins of life on Earth.

Launched in 1997, the internationally produced Cassini-Huygens spacecraft reached its large, gaseous destination in July 2004, with contributions from UCLA scientists and alumni. Onboard, a suite of 12 instruments that includes a radio antenna, magnetic field detector, dust collector and cameras photographing the planet and its moons in various light wavelengths send data back to Earth.

“A major goal of studying planets is to discover how the solar system came into being, and Cassini is no exception,” said Krishan Khurana, a professor of space physics at UCLA who was consulted by the team of UCLA scientists working on Cassini’s magnetic field detector. The team was headed by Christopher Russell, a professor of geophysics and planetary physics at UCLA.

“(Studying magnetic fields) tells us about the internal space, the core material, of the planet,” Khurana said.

Magnetic fields are created by many planets in our solar system, including Earth, Khurana said.

He explained that they help stabilize the surface of a planet by protecting it from solar wind – particles (electrons) that the sun sends out into the solar system – which would otherwise strip away the atmosphere.

“Now for the first time, Cassini will map this (magnetic) field from various latitudes,” Khurana said.

In addition, an in-depth study of Saturn’s ring system may illuminate the origins of the solar system, said Linda Spilker, deputy project scientist for Cassini and UCLA alumna.

Spilker added that Saturn’s rings, composed of chunks of ice and dirt, orbit the planet like grooves on a phonograph record and are a good analogy for the larger solar system: The rings may have been created similar to the way the planets gathered around the Sun.

“It may be that by studying Saturn’s rings, we will learn how planets formed,” Spilker said.

The second part of the Cassini mission involves a trip to the surface of Saturn’s biggest moon, Titan, which is larger than the planet Mercury.

“If it had formed elsewhere in the solar system, it would have been a planet,” Spilker said of Titan.

The Huygens probe will be launched from the Cassini spacecraft on Dec. 24 and will enter Titan’s atmosphere in January 2005, with hopes of discovering how life might have evolved on Earth.

Previous observations have shown scientists that smog-forming materials, such as methane and ethane, compose Titan’s thick atmosphere, comparable to what scientists believe existed on early Earth over 4 billion years ago.

By studying Titan further, scientists hope to better understand how early our planet’s atmosphere evolved, Khurana said.

“The atmosphere is very close to Earth’s atmosphere – enough that we’d like to understand it,” Khurana said.

During its parachute-assisted dive to the surface, the Huygens probe will measure temperature, wind velocity and pressure changes in Titan’s atmosphere.

The probe’s fins will cause it to spin while falling, so that its three cameras create a giant panorama view of the foreign moon.

There is even a microphone to record Titan’s sounds, and a light will ignite just before the Huygens probe reaches the surface, like the “flash” of a camera, allowing the device to send back detailed pictures of the surface.

Scientists hope the probe will finally determine whether Titan’s surface contains liquid and whether that liquid holds the oxygen that is necessary for life.

“The biggest mystery about Titan is, we still don’t know what its surface is composed of,” Khurana said. “We would love to know if there is ice on the surface, and the quantity of the ice.”

Spilker said Cassini will study Saturn for at least four years, providing scientists with a more detailed picture of the planet and its surrounding moons than any of the three previous Saturn-viewing missions.