Discovery of smallest planet yet a 'milestone' in search for another Earth
The Kepler space telescope has found a planet smaller than Mercury orbiting a distant star. The discovery suggests Kepler has the precision to find a planet more like Earth.
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Just as geophysicists can use earthquake vibrations traveling through the Earth to reconstruct the planet's interior, astrophysicists can use the same approach for determining the structure of distant stars. Kepler takes the measure of a star by recording rapid changes in its brightness from what in essence are sound waves moving through the hot gas.Skip to next paragraph
In Pictures Looking into the skies: Telescopes
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In some cases, Kepler's insight into a star has forced team members to boost the size and mass estimates of its planets. These revisions mean planets that were initially thought to be comparable in size and mass to Earth, often turn out not to be rocky planets in all likelihood, Barclay explains.
So when Barclay took his data suggesting a tiny planet to the Kepler mission's resident astroseismologist, the colleague was not optimistic. "But then he came running down the corridor saying: 'I've detected something!' " Barclay recalls. Extremely precise measurements of the star Kepler 37 indicated that it indeed was relatively small star, hence the initial estimate of Kepler 37b as a munchkin held up.
Unfortunately, independent efforts to confirm the planet's presence with Earth-based telescopes using a different detection approach – which spots the wobble a star's spectrum displays from the gravitational tug of an orbiting planet – came up empty.
Still, the Kepler team was able to rule out other possible explanations for Kepler 37's dimming to a high degree of confidence using statistical tools and the long observations of the star and its cosmic neighborhood.
Computer simulations suggest that the planet and its two siblings are in a stable configuration around the star, and that the planet likely is rocky and devoid of an atmosphere. The simulations also indicated that Kepler 37b would have swept its orbital zone clear of any debris left over from the system's formation some 6 billion years ago. This puts it squarely in the "planet" camp, despite its diminutive size, versus "dwarf planet," the category to which Pluto has been exiled.
"This is a hot planet on a short orbit," Barclay says. "The next step is to look for planets on longer orbital periods. It's just a matter of time. The longer you look, the further out in orbital period you can probe."
But he's not undervaluing this discovery.
"The fact that we are finding things smaller than we know of in our own solar system I think is really exciting," he says. "We're probing the architectures of other star systems."