The Hobby=Eberly Telescope, one of the world's largest, will work with NASA's Kepler spacecraft to find Earth-like planets.
Texas telescope to help spot Earth-like planets
13 Mar 2009
University of Texas at Austin astronomer Bill Cochran is one of the leading scientists involved in searching 100,000 nearby stars in our Milky Way galaxy for planets like Earth as part of NASA's Kepler mission.
The Kepler mission spacecraft launched aboard a Delta-II rocket on March 7 (Sydney time).
Results from Kepler's 3.5-year mission will allow scientists to place our solar system in context with other planetary systems in the Milky Way galaxy.
The Kepler mission is equipped with a scientific instrument called a photometer, or light meter. It will monitor the brightness of its 100,000 target stars within a single field of view steadily for 3.5 years, looking for periodic dips in their brightness. These dips might indicate an orbiting planet passing in front of the star, an event called a "transit."
Once Kepler finds a probable planet, that's where Cochran comes in.
"My role is part of the Follow-up Observations Group," he said. "When [Kepler] detects a transit of a planet around a star, our job is to use other facilities to find out as much as possible about the planet and the star itself. I'll go out to HET," referring to the Hobby-Eberly Telescope at the University's McDonald Observatory in West Texas.
Cochran will use HET, one of the world's largest telescopes, to closely monitor the motions of the target star. These observations, combined with the data from Kepler, will determine the planet's mass, a critical factor in determining how similar the planet is to Earth.
A star's Goldilocks zone is where the temperature is right for liquid to exist—not too hot, nor too cold.
Of the nearly 350 planets found orbiting stars other than the Sun to date, none have been found with masses as low as Earth's—yet. That's not necessarily due to a lack of Earth-mass planets in our galaxy. It may be simply due to our technological limitations.
"We're going to try to push down the mass," Cochran said. "Finding a planet with the mass of Earth is very, very hard."
Cochran's follow-up observations might also detect other planets orbiting these stars. If such planets do not transit in front of the star, they will not be seen by Kepler, but should be detectable through Cochran's observing technique with HET. Called "radial velocity," the technique involves monitoring the star's motion toward and away from Earth to detect any wobbles due to the presence of orbiting planets.
Fellow University of Texas at Austin astronomer Don Winget is also involved in the Kepler mission. He will use Kepler's measurements of stars' light output over time as way to "see inside" these stars and measure their internal structure—the same way geologists use sound waves to "see inside" Earth. In geology, the technique is called seismology. In astronomy, it's referred to as "asteroseismology."
The Kepler mission's main goal is to determine the number of Earth-like planets in the Milky Way galaxy, and to understand the characteristics of these planetary systems. With Cochran using McDonald Observatory's giant Hobby-Eberly Telescope to measure these stars' orbits, confirm orbiting planets and discover new ones, and Winget and his team studying the deep interiors of the stars to determine their structure, composition, and ages, The University of Texas at Austin will make a major contribution to Kepler's success.
Adapted from information issued by McDonald Observatory / Marty Harris / UT-Austin.
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