Abstract
More than 200 extrasolar planets have been discovered around relatively nearby stars, primarily through the Doppler line shifts owing to reflex motions of their host stars, and more recently through transits of some planets across the faces of the host stars. The detection of planets with the shortest known periods, 1.2–2.5 days, has mainly resulted from transit surveys which have generally targeted stars more massive than 0.75 M⊙, where M⊙ is the mass of the Sun. Here we report the results from a planetary transit search performed in a rich stellar field towards the Galactic bulge. We discovered 16 candidates with orbital periods between 0.4 and 4.2 days, five of which orbit stars of masses in the range 0.44–0.75 M⊙. In two cases, radial-velocity measurements support the planetary nature of the companions. Five candidates have orbital periods below 1.0 day, constituting a new class of ultra-short-period planets, which occur only around stars of less than 0.88 M⊙. This indicates that those orbiting very close to more-luminous stars might be evaporatively destroyed or that jovian planets around stars of lower mass might migrate to smaller radii.
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Acknowledgements
This article is based on observations made with the NASA/ESA Hubble Space Telescope, obtained at the Space Telescope Science Institute, which is operated by the AURA, Inc. under a NASA contract, and with the Very Large Telescope at the ESO, Paranal, Chile. We thank R. Gilliland for his generous contribution of time and efforts for this project, and D. Bradstreet, I. Jordan, G. Kovacs, D. VandenBerg and the late A. Lubenow for their help at various stages of the project.
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Supplementary Figures Legends
This file contains text to accompany the below Supplementary Figures. (DOC 21 kb)
Supplementary Figure 1a
Full-resolution transit light curves. (JPG 96 kb)
Supplementary Figure 1b
Full-resolution transit light curves. (JPG 90 kb)
Supplementary Figure 1c
Full-resolution transit light curves. (JPG 96 kb)
Supplementary Figure 1d
Full-resolution transit light curves. (JPG 96 kb)
Supplementary Figure 2a
Binned transit light curves. (JPG 82 kb)
Supplementary Figure 2b
Binned transit light curves. (JPG 74 kb)
Supplementary Figure 2c
Binned transit light curves. (JPG 79 kb)
Supplementary Figure 2d
Binned transit light curves. (JPG 80 kb)
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Sahu, K., Casertano, S., Bond, H. et al. Transiting extrasolar planetary candidates in the Galactic bulge. Nature 443, 534–540 (2006). https://doi.org/10.1038/nature05158
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DOI: https://doi.org/10.1038/nature05158
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