Astronomers Catch Planet By Unusual Means
Baltimore MD (SPX) May 19, 2006
An international team of professional and amateur astronomers, using simple off-the-shelf equipment to trawl the skies for planets outside the solar system, has hauled in their first catch.
The astronomers discovered a Jupiter-sized planet orbiting a Sun-like star 600 light-years away in the constellation Corona Borealis, or the Northern Crown.
Using modest telescopes to search for extrasolar planets allows for a productive collaboration between professional and amateur astronomers that could accelerate the planet quest.
"This discovery suggests that a fleet of modest telescopes and the help of amateur astronomers can search for transiting extrasolar planets many times faster than we are now," said team leader Peter McCullough of the Space Telescope Science Institute.
McCullough deployed a relatively inexpensive telescope made from commercial equipment to scan the skies for extrasolar planets. Called the XO telescope, it consists of two 200 millimeter telephoto camera lenses and looks like a pair of binoculars. The telescope is on the summit of the Haleakala volcano, on the island of Mau`i, Hawaii.
"To replicate the XO prototype telescope would cost $60,000," McCullough explained. "We have spent far more than that on software, in particular on designing and operating the system and extracting this planet from the data."
McCullough's team found the planet, which they call X0-1b, by noticing slight dips in the star's light output when the planet transited the star. The light from the star, called XO-1, dips by approximately 2 percent when the planet XO-1b passes in front of it. The observation also revealed X0-1b circles the star in a tight four-day orbit.
Astronomers have detected more than 180 extrasolar planets to date, but X0-1b is only the tenth discovered using the transit method, and only the second found using telephoto lenses. The first, dubbed TrES-1, was reported in 2004. The transit method allows astronomers to determine a planet's mass and size. Astronomers use this information to deduce the planet's characteristics, such as its density.
The team confirmed the planet's existence by using the Harlan J. Smith Telescope and the Hobby-Eberly Telescope at the University of Texas's McDonald Observatory to measure the slight wobble induced by the planet on its parent star. This method, called radial velocity, allowed the team to calculate a precise mass for the planet, which is slightly less than that of Jupiter (about 0.9 Jupiter masses).
The planet also is much larger than its mass would suggest. "Of the planets that pass in front of their stars, XO-1b is the most similar to Jupiter yet known, and the star XO-1 is the most similar to the Sun," McCullough said. "But XO-1b is much, much closer to its star than Jupiter is to the Sun."
The technique of using relatively inexpensive telescopes to look for eclipsing planets favors finding planets orbiting close to their parent stars. The planet also must be large enough to produce a measurable dip in starlight.
McCullough's planet-finding technique involves nightly sweeps of the sky using the XO telescope in Hawaii to note the brightness of the stars it encounters. A computer software program sifts through many thousands of stars every two months looking for tiny dips in the stars' light, the signature of a possible planetary transit.
The computer generates a few hundred possibilities. From those candidates, McCullough selects a few dozen promising leads, which he passes on to team members to study the possible transits more carefully.
From September 2003 to September 2005, the XO telescope observed tens of thousands of bright stars. In that time, the team studied a few dozen promising candidate stars. The star X0-1 was pegged as a promising candidate in June 2005.
The team observed it in June and July 2005, confirming that a planet-sized object was eclipsing the star. McCullough then turned to the McDonald Observatory in Texas to obtain the object's mass and verify it as a planet. He received the news of the telescope's observation at 12:06 a.m. Feb. 16, 2006, from Chris Johns-Krull, a friend and colleague at Rice University.
"It was a wonderful feeling because the team had worked for three years to find this one planet," McCullough explained. "The discovery represents a few bytes out of nearly a terabyte of data: It's like trying to distill gold out of seawater."
McCullough said he thinks the newly found planet is a perfect candidate for study by the Hubble and Spitzer space telescopes. Hubble can measure precisely the star's distance and the planet's size. Spitzer actually can see the infrared radiation from the planet.
By timing the disappearance of the planet behind the star, Spitzer also can measure the "ellipticity," or "out-of-roundness," of the planet's orbit. If the orbit is elliptical, then the varying gravitational force would result in extra heating of the planet, expanding its atmosphere and perhaps explaining why the object's diameter seems especially large for a body of its calculated mass.
"By timing the planet's passages across the star, both amateur and professional astronomers might be lucky enough to detect the presence of another planet in the XO-1 system by its gravitational tugs on XO-1b," McCullough said. "It's even possible that such a planet could be similar to Earth."
McCullough's team includes four amateur astronomers from North America and Europe. Their account of the discovery has been accepted for publication in the Astrophysical Journal.
Space Telescope Science Institute
Simulation Tracks Planetary Evolution
London, UK (SPX) Mar 21, 2006
Two British astronomers have constructed a computer simulation that tracks how giant protoplanets tend to form and migrate inward toward their central star.
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