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Detection of Planetary Transits Across a Sun-like Star
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We report high-precision, high-cadence photometric measurements of the star HD 209458, which is known from radial velocity measurements to have a planetary-mass companion in a close orbit. We detect two separate transit events at times that are consistent with the radial velocity measurements. In both cases, the detailed shape of the transit curve due to both the limb darkening of the star and the finite size of the planet is clearly evident. Assuming stellar parameters of 1.1 R middle dot in circle and 1.1 M middle dot in circle, we find that the data are best interpreted as a gas giant with a radius of 1.27+/-0.02 RJup in an orbit with an inclination of 87&fdg;1+/-0&fdg;2. We present values for the planetary surface gravity, escape velocity, and average density and discuss the numerous observations that are warranted now that a planet is known to transit the disk of its parent star.
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“A number of hot Jupiters-including HD 209458b, the first hot Jupiter to be discovered to transit (Charbonneau et al. 2000, Henry et al. 2000)-have radii larger than expected from internal structure models.”
From Origins of Hot Jupiters (2018) · cites this paper as Charbonneau et al. 2000
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Metadata
- Authors
- Charbonneau, D., Brown, T. M., Latham, D. W., & Mayor, M.
- Affiliations
- NSF National Center for Atmospheric Research (US)
- Center for Astrophysics Harvard & Smithsonian (US)
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2000-01-20
- Volume
- 529
- Issue
- 1
- Pages
- L45-L48
- ISSN
- 0004-637X (ISSN-L)
- OpenAlex
- W2151864661
- Cited by
- 1,415
- References
- 14
- Citations by year
- 2026: 25 · 2025: 44 · 2024: 48 · 2023: 50 · 2022: 42 · 2021: 36 · 2020: 60 · 2019: 50 · 2018: 60 · 2017: 54 · 2016: 55 · 2015: 42 · 2014: 39 · 2013: 56 · 2012: 49
- FWCI
- 48.04
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- PubMed (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- Digital Access to Scholarship at Harvard (DASH) (Harvard University) (submittedVersion, cc-by)
- arXiv (Cornell University)
- Funders
- National Aeronautics and Space Administration
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Instrumentation › Astronomy and Astrophysical Research
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
- Keywords
- HD 209458, planetary transits, exoplanets, hot Jupiters, transit photometry, limb darkening, transit timing, orbital inclination, planetary radius, surface gravity, escape velocity, planet density, solar-type stars
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