An extrasolar planet that transits the disk of its parent star

Maciej Konacki (), Guillermo Torres, Saurabh Jha and Dimitar D. Sasselov
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Maciej Konacki: California Institute of Technology
Guillermo Torres: Harvard-Smithsonian Center for Astrophysics
Saurabh Jha: Harvard-Smithsonian Center for Astrophysics
Dimitar D. Sasselov: Harvard-Smithsonian Center for Astrophysics

Nature, 2003, vol. 421, issue 6922, 507-509

Abstract: Abstract Planets orbiting other stars could in principle be found through the periodic dimming of starlight as a planet moves across—or ‘transits’—the line of sight between the observer and the star. Depending on the size of the planet relative to the star, the dimming could reach a few per cent of the apparent brightness of the star. Despite many searches, no transiting planet has been discovered in this way; the one known1,2 transiting planet—HD209458b—was first discovered using precise measurements2,3 of the parent star's radial velocity and only subsequently detected photometrically. Here we report radial velocity measurements of the star OGLE-TR-56, which was previously found to exhibit a 1.2-day transit-like light curve4,5 in a survey looking for gravitational microlensing events. The velocity changes that we detect correlate with the light curve, from which we conclude that they are probably induced by an object of around 0.9 Jupiter masses in an orbit only 0.023 au from its star. We estimate the planetary radius to be around 1.3 Jupiter radii and its density to be about 0.5 g cm-3. This object is hotter than any known planet (∼ 1,900 K), but is still stable against long-term evaporation or tidal disruption.

Date: 2003
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DOI: 10.1038/nature01379

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