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One of two sets of cameras known as SuperWASP. The batteries hunt for extrasolar planets by looking for transits among millions of stars at a time. Credit: SuperWASP |
Astronomers have struggled for centuries to find our solar system's planets, let alone any outside of our relatively puny cosmic neighborhood.
Yet during only the past 13 years, observers have tracked down nearly 300 distant bodies beyond our system thanks to rapid advances in ground-based telescope technology and methods.
Ten worlds alone were identified by a group of astronomers in the past six months using earthbound instruments, and another team of scientists just announced they have found the youngest-ever planetary infant. The hunt for the first Earth-like planet, however, is still on.
Observers discussed the state of their search for extrasolar planets, as worlds beyond the solar system are known, during the Royal Astronomical Society's National Astronomy Meeting in Belfast, U.K., this week.
Sting operation
Extrasolar planets are tough for telescopes to detect unless the objects are about the size of Jupiter, which is why astronomers rely on unique methods to find the elusive bodies.
Periodic wiggles in stellar movement can signal an orbiting world's gravitational tug on its star. Another method looks for dips in stellar brightness called transits ? when planets pass directly in front of a star and block out some of the light.
Instead of spending weeks babysitting single stars to seek out gravitational wiggles, as many planet-hunters do, some European astronomers are monitoring millions of stars with inventive camera setups such as one called SuperWASP.
?SuperWASP is now a planet-finding production line," said Don Pollacco, a SuperWASP project member and a Queen?s University Belfast (QUB) astronomer.
In the past six months alone, Pollacco said, the project's two batteries of cameras in South Africa and the Canary Islands have pinpointed 10 new planets, for which SuperWASP has also estimated size and mass.
"[It] will revolutionize the detection of large planets and our understanding of how they were formed," Pollacco said of the new planet-hunting program. "It?s a great triumph for European astronomers.?
Fetal planet
In addition to the 10 new extrasolar recruits ? the comprehensive exoplanet count now totals 277 ? another group of astronomers said they've located an embryonic star younger than any seen before with the Very Large Array of radio telescopes in New Mexico.
The group, led by Jane Greaves of the University of St. Andrews in Scotland, found the 100,000-year-old fetal planet about 520 light-years away in the constellation Taurus
?The new object, designated HL Tau b, is the youngest planetary object ever seen," said Anita Richards, an astronomer at the U.K. Jodrell Bank Centre for Astrophysics.
Richards, who worked with Greaves' team to describe the infant planet, said it's just 1 percent as old as the young planet found in orbit around the star TW Hydrae last year.
"We see a distinct orbiting ball of gas and dust, which is exactly how a very young protoplanet should look," Greaves said, noting the far-younger planet should take on a Jupiter-like essence in millions of years.
Another Earth?
Although astronomers are developing large, space-based projects to hunt for Earth-like planets ? such as the Jet Propulsion Lab's proposed Terrestrial Planet Finder ? ground-based observers aren't sitting idly by.
In hopes of finding small rocky planets, some U.K. astronomers are using a special camera known as "RISE" that is mounted onto the Liverpool Telescope in England. The device rapidly photographs a portion of the sky and compares the brightness of stars and large extrasolar planets from image to image.
If there's any dimming, said Neale Gibson, also a QUB astronomer, the instrument will find it and reveal if small rocky planets are disturbing the orbits of hot, gassy planets.
"RISE will allow us to observe and time the transits of extrasolar planets very accurately," Gibson said. "If Earth-mass planets are present in nearby orbits ? we will see their effect on the orbit of the larger transiting planets.?
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