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Update: Boss and Seager Comment on Puzzling Planets |
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Tuesday, 19 September 2006 |
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Alan Boss is quoted in a Science News online article entitled, “Oversize Orb: Puffy planet poses puzzle.” The article discusses HAT-P-1b, an object located 450 light-years from Earth that may be the largest planet found to date. According to the Harvard-Smithsonian Center for Astrophysics team, the planet is 36 percent greater in diameter than Jupiter and resides just one-twentieth the distance from its parent star than Earth is from the Sun.
The object was detected because it passes directly between its parent star, the fainter of a double-star system called ADS 16402, and the Earth about every two hours. During these transits, the planet blocks 1.5 percent of the star’s light from reaching the Earth. HAT-P-1b is the twelfth of the 200 extrasolar planets to be observed transiting across its star.
Only one other transiting planet, HD 209458b, has a density nearly as low as that of HAT-P-1b, and some researchers had regarded HD 209458b as a fluke. Boss comments, “Puffy hot Jupiters do not appear to be as rare as one might have been able to argue before this discovery.” The full article can be accessed here.
More on Puffy Planets: Seager Comments
Sara Seager is quoted in a New Scientist Space article entitled, “Third ‘puffed-up planet’ discovered" that discusses WASP-1b, the first planet to be discovered by the Super Wide Angle Search for Planets (SuperWASP), led by Queen’s University, Belfast. This planet is the third planet of extremely low density to be discovered by transit technique. Seager commented, “Finding more examples of puffed-up planets could help astronomers solve the puzzle of what makes them bloat. Having a third low-density hot Jupiter can help us evaluate how rare that scenario is.”
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