Jupiter's moon Europa should be NASA's next target, says ASU researcher
Greeley, a Regents' Professor, heads the Planetary Geology Group in ASU's School of Earth and Space Exploration. He presented the Europa proposal Feb. 18 at the annual meeting of the American Association for the Advancement of Science in San Francisco.
"Europa is unique in our solar system," says Greeley. "It's a rocky object a little smaller than our Moon, and it's covered with a layer of water 100 miles deep." This holds more water than all the oceans on Earth, he explains. Greeley adds that Europa also has the two other basic ingredients of life -- organic chemistry and a source of energy.
Scientists have identified four candidate worlds beyond Earth that might contain life, either now or in the past, Greeley says. These four are Mars, Saturn's moons Titan and Enceladus, and Jupiter's moon Europa.
Mars is the target of numerous ongoing missions, and NASA's Cassini spacecraft is studying both Titan and Enceladus at present. Cassini's results, however, show that Titan and Enceladus have temperatures hundreds of degrees Fahrenheit below zero and may not hold any liquid water.
"We know Europa's surface is frozen," Greeley says. "But we don't know if it's frozen all the way down, or if there's an ocean under an ice shell."
The ice thickness is a key question, notes Greeley.
"Ultimately, we want to get down through that ice shell and into the ocean where any action is," he says. "So it matters whether the ice is 10 yards thick, or 10 miles or more. The data we have today will never answer that question."
Europa's place in the Jovian system, however, provides a possible means of measuring the ice shell's thickness. As Europa circles Jupiter every 3.6 days, it orbits in lockstep with two other moons, Ganymede and Callisto. The gravity of these bodies, plus Jupiter itself, raises tides in Europa that heat it by friction.
"Geophysical models show that if the ice goes all the way down, the amount of tidal flexing will be small, only a few feet or so," Greeley explains. "But if the ice shell is thin, say 30 feet thick, the tidal flexing could range 130 feet." What's needed, Greeley adds, is an instrument that can measure the flexing on a continuing basis.
Mission details still need to be developed, Greeley notes, along with basic specifications for instruments and performance. He is working with Robert Pappalardo, an ASU graduate now at the Jet Propulsion Laboratory, to define more carefully the Europa orbiter mission. They expect to finish their work by the end of this summer.
The U.S. National Academy of Sciences published a report in 2003 summarizing what planetary scientists felt were the highest priority missions for the decade ahead. A Europa geophysical mission stood at the top of the list.
"In the minds of many researchers," says Greeley, "Europa is of primary importance."