Finding Planets Is Job One: Explaining Them Is Next

By Robert C. Cowen, Monitor | The Christian Science Monitor, January 19, 1996 | Go to article overview
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Finding Planets Is Job One: Explaining Them Is Next

Robert C. Cowen, Monitor, The Christian Science Monitor

PLANET-HUNTING astronomers have crossed a watershed. Encouraged by detection of Jupiter-class planets orbiting sun-like stars, they are turning from mere hopeful exploration to the more demanding task of gaining a deeper understanding of how planetary systems form.

"We're at a turning point ... we're {actually} finding new worlds!" exclaims William Borucki of the NASA/Ames Research Center in Mountain View, Calif. "We're going from the discovery phase to trying to understand the science," explains William Cochran of the University of Texas at Austin.

Yet the challenge now is to find examples of more extensive planetary systems, says David Black, director of the Lunar and Planetary Institute in Houston. Scientists need analogs of our own solar system's suite of multiple planets to test their theories, he said. He expects the recent discoveries to spur on efforts to do this.

Such is the impact of Wednesday's report to a meeting of the American Astronomical Society that Geoffrey Marcy of San Francisco State University and Paul Butler of the University of California at Berkeley have detected two Jupiter-size planets that could support liquid water. They orbit the stars 70 Virginis in the constellation Virgo and 47 Ursae Majoris in the Big Dipper.

This gives astronomers three examples of such planetary systems to whet their scientific appetites. The third example - a Jupiter-class planet orbiting 51 Pegasi in the constellation Pegasus - was reported last October by Michel Mayor and Didier Queloz of the Geneva Observatory in Switzerland. Drs. Black, Borucki, and Cochran joined several other astronomers in briefing the press on new possibilities to add to this list.

So far, the best clue to a planet's presence has been its gravitational interaction with its parent star. This causes the star to wobble in a way that reveals the planet's size and orbit. That's the method Marcy, Butler, and the Swiss astronomers used. While this technique is being refined, other methods are becoming practical.

For example, Borucki explained that even Earth-size planets can be detected by the way they dim a star's light when they move in front of the star's disk.

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Finding Planets Is Job One: Explaining Them Is Next


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