Tatooine Times Two: Amateur Astronomers Find Planet in Four-Star System
http://www.wired.com/wiredscience/2012/10/planet-hunters-four-star/

A group of volunteers using a citizen science astronomy website have discovered 
an extrasolar planet orbiting a record four stars.

Scarcely a year ago, astronomers weren’t sure if planets could exist in binary 
star systems, where two stars orbit one another. But after the discovery of a 
circumbinary exoplanet - which would have two suns in its sky, much like the 
famous Tatooine of Star Wars - scientists realized that such worlds were 
possible and have found at least five more similar systems. About half of stars 
in the universe are found in binary pairs and if they can host planets then the 
chances for life outside our own world may be greatly increased.

The newly discovered exoplanet orbits within a quadruple star system named KIC 
4862625 that is about 3,200 light-years from Earth. Citizen scientists Kian Jek 
of San Francisco and Robert Gagliano of Cottonwood, Arizona, used the website 
Planethunters.org to scan data from these stars captured by NASA’s Kepler space 
telescope and noticed a periodic dip in their light.

The data showed that a planet was passing in front of its parent stars, a 
binary pair, every 138 days and eclipsing their light. The planet has been 
dubbed PH1 (Planet Hunters 1) and is estimated to be a gas giant with a radius 
6.2 times that of Earth, making it slightly bigger than Neptune, and a mass 
roughly half that of Jupiter. The binary stars have about 1.5 and 0.41 times 
the mass of the sun and orbit one another with a period of 20 days.

PH1′s binary pair parents are in turn orbited by another binary pair of stars 
at a distance 1,000 times that between the Earth and the sun. If any beings 
could live on PH1, they would not only witness a double sunset but might also 
be able to spot two bright stars in their night sky wandering against the 
background stars.

The work was confirmed by astronomers at Yale. It is being presented Oct. 15 at 
the American Astronomical Society’s Division for Planetary Sciences meeting in 
Reno, Nevada and has been submitted to The Astrophysical Journal for 
publication.
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