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Cited by 237Stellar, planetary, and galactic studiesAstro and Planetary ScienceIonosphere and magnetosphere dynamics

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The effect of tidal locking on the magnetospheric and atmospheric evolution of “Hot Jupiters”

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Grießmeier, J.-M., Stadelmann, A., Penz, T., Lammer, H., Selsis, F., Ribas, I., Guinan, E. F., Motschmann, U., Biernat, H. K., Weiss, W. W.·2004·Astronomy & Astrophysics
DOI 10.1051/0004-6361:20035684
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Abstract

We study the interaction between the planetary magnetosphere and atmosphere of the close-in extrasolar planets HD 209458b and OGLE-TR-56b with the stellar wind during the evolution of their host stars. Recent astrophysical observations of solar-like stars indicate that the radiation and particle environments of young stars are orders of magnitudes larger than for stars with ages comparable to the sun (~4.6 Gyr). We model the interaction for the present and for early evolutionary stages, showing that it is possible that “Hot Jupiters” have an ionosphere-stellar wind interaction like Venus. Our study suggests that the internal magnetic field of exoplanets orbiting close to their host stars may be very weak due to tidal locking. The magnetic moments can be less than one tenth of the value presently observed for the rapidly rotating planet Jupiter. We find that the stronger stellar wind of younger solar-type stars compresses the magnetosphere to a standoff distance at which the ionized part of the upper atmosphere, hydrodynamically expanded by the XUV-flux, builds an obstacle. Because of a much larger stellar wind particle flux during the first ~0.5 Gyr after the host stars arrived on the Zero-Age-Main-Sequence, “Hot Jupiters” may have not been protected by their intrinsic magnetic fields, even if one neglects the effect of tidal locking. In such a case, the unshielded upper atmosphere will be affected by different ionization and non-thermal ion loss processes. This contributes to the estimated neutral hydrogen loss rates of about ≥ of the observed expanded exosphere of HD 209458b [CITE] and will be an ionized part of the estimated upper energy-limited neutral hydrogen loss rates of about [CITE].

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  • Unless a hosted CLI-HZ planet has a strong and persistent magnetic field, there is a significant possibility that the planet will lose most, if not all, of its atmosphere including its water inventories.

    “Unless a hosted CLI-HZ planet has a strong and persistent magnetic field, amounting to a protective magnetosphere, there is a significant possibility that the planet will lose most, if not all, of its atmosphere including its water inventories (e.g., Grießmeier et al. 2004).”

    From ABOUT EXOBIOLOGY: THE CASE FOR DWARF K STARS (2016) · cites this paper as Grießmeier et al. 2004

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Metadata

Authors
Grießmeier, J.-M., Stadelmann, A., Penz, T., Lammer, H., Selsis, F., Ribas, I., Guinan, E. F., Motschmann, U., Biernat, H. K., & Weiss, W. W.
Affiliations
  • Technische Universität Braunschweig (DE)
  • Austrian Academy of Sciences (AT)
  • Consejo Superior de Investigaciones Científicas (ES)
  • Institute of Space Sciences (ES)
  • Villanova University (US)
  • University of Vienna (AT)
ORCID
Venue
Astronomy & Astrophysics
Publisher
EDP Sciences
Published
2004-09-21
Volume
425
Issue
2
Pages
753-762
ISSN
  • 0004-6361 (ISSN-L)
  • 1432-0746
DOI
10.1051/0004-6361:20035684
OpenAlex
W2054674651
Cited by
237
References
2
Citations by year
2026: 4 · 2025: 5 · 2024: 9 · 2023: 3 · 2022: 5 · 2021: 4 · 2020: 8 · 2019: 4 · 2018: 38 · 2017: 11 · 2016: 11 · 2015: 8 · 2014: 11 · 2013: 7 · 2012: 7
FWCI
8.85
Type
journal article
Language
en
Open access
Locations
  • Astronomy and Astrophysics (publishedVersion)
  • Springer Link (Chiba Institute of Technology) (submittedVersion)
  • HAL (submittedVersion, other-oa)
Funders
  • National Aeronautics and Space Administration (NAG510387, NAG512125)
  • Austrian Science Fund (P17099, P 14984)
  • Karl-Franzens-Universität Graz
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 › Earth and Planetary Sciences › Space and Planetary Science › Ionosphere and magnetosphere dynamics
Keywords
tidal locking, hot Jupiters, planetary magnetospheres, stellar winds, exoplanet atmospheres, HD 209458b, stellar evolution, stellar magnetic fields, ionospheric escape, XUV radiation, exosphere

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