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    A Planet So Light It Would Float on Water

    Astronomers have found a strange new planet which is so puffy it would float on
    water.

    The new planet, designated HAT-P-1, orbits one member of a pair of distant
    stars 450 light-years away in the constellation Lacerta.

    Gaspar Bakos, a Hubble fellow
    at the Harvard-Smithsonian
    Center for Astrophysics (CfA)
    and lead author of a paper
    submitted to the Astrophyical
    Journal detailing the discovery,
    says the planet is lighter than a
    giant ball of cork.

    "It would float in a bathtub if you
    could find a tub big enough to
    hold it, " he said.

    Bakos said it's unlike any world
    known to science.
    The mysterious planet as seen in this lllustration   
    by David A. Aguilar (CfA)

    "We could be looking at an entirely new class of planets," he said.

    With a radius about 1.38 times Jupiter's, HAT-P-1 is the largest known planet.
    In spite of its huge size, its mass is only half that of Jupiter.

    HAT-P-1 revolves around its host star every 4.5 days in an orbit one-twentieth of
    the distance from Earth to the Sun.  Its parent star is one member of a double-
    star system called ADS 16402 and is visible in binoculars.

    The two stars are separated by about 1500 times the Earth-Sun distance. They
    are similar to the Sun but slightly younger - about 3.6 billion years old
    compared to the Sun's age of 4.5 billion years.

    Although stranger than any other extrasolar planet found so far, HAT-P-1 is not
    alone in its low-density status. The first planet ever found to transit its star, HD
    209458b, also is puffed up about 20 percent larger than predicted by theory.
    HAT-P-1 is 24 percent larger than expected.

    "Out of eleven known transiting planets, now not one but two are substantially
    bigger and lower in density than theory predicts," said co-author Robert Noyes
    (CfA). "We can't dismiss HD209458b as a fluke. This new discovery suggests
    something could be missing in our theories of how planets form."
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