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CALIBRATION OF EQUILIBRIUM TIDE THEORY FOR EXTRASOLAR PLANET SYSTEMS
Open accessAbstract
We provide an "effective theory" of tidal dissipation in extrasolar planet systems by empirically calibrating a model for the equilibrium tide. The model is valid to high order in eccentricity and parameterized by two constants of bulk dissipation—one for dissipation in the planet and one for dissipation in the host star. We are able to consistently describe the distribution of extrasolar planetary systems in terms of period, eccentricity, and mass (with a lower limit of a Saturn mass) with this simple model. Our model is consistent with the survival of short-period exoplanet systems, but not with the circularization period of equal mass stellar binaries, suggesting that the latter systems experience a higher level of dissipation than exoplanet host stars. Our model is also not consistent with the explanation of inflated planetary radii as resulting from tidal dissipation. The paucity of short-period planets around evolved A stars is explained as the result of enhanced tidal inspiral resulting from the increase in stellar radius with evolution.
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Tidal heating shuts off as the orbit nears circularization, so stellar irradiation mechanisms could take over at that point.
“Tidal heating shuts off as the orbit nears circularization (e.g., Leconte et al. 2010, Hansen 2010), so stellar irradiation mechanisms could take over at that point.”
From Origins of Hot Jupiters (2018) · cites this paper as Hansen 2010
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WASP-17b: AN ULTRA-LOW DENSITY PLANET IN A PROBABLE RETROGRADE ORBIT
Anderson, D. R., Hellier, C., Gillon, M., Triaud, A. H. M. J., Smalley, B., Hebb, L., Cameron, A. C., Maxted, P. F. L., Queloz, D., West, R. G., et al. (2010) · The Astrophysical Journal · doi:10.1088/0004-637x/709/1/159 · Cited by 208
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Cited by
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Dawson, R. I., & Johnson, J. A. (2018) · Annual Review of Astronomy and Astrophysics · doi:10.1146/annurev-astro-081817-051853 · Cited by 622
Metadata
- Authors
- Hansen, B. M. S.
- Affiliations
- University of California, Los Angeles (US)
- Corresponding author
- Hansen, Brad M. S.
- ORCID
- Hansen, Brad M. S.
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2010-10-08
- Volume
- 723
- Issue
- 1
- Pages
- 285-299
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W4237204345
- Cited by
- 173
- References
- 1
- Citations by year
- 2026: 11 · 2025: 11 · 2024: 3 · 2023: 5 · 2022: 13 · 2021: 11 · 2020: 11 · 2019: 10 · 2018: 11 · 2017: 12 · 2016: 10 · 2015: 11 · 2014: 11 · 2013: 10 · 2012: 20
- FWCI
- 7.69
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- arXiv (Cornell University)
- Topics
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
- Keywords
- equilibrium tide, tidal dissipation, exoplanets, orbital circularization, stellar evolution, A-type stars, short-period planets, binary stars, eccentricity
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