Cited by 172Stellar, planetary, and galactic studiesAstronomy and Astrophysical ResearchHistory and Developments in Astronomy

The oblique orbit of the super-Neptune HAT-P-11b

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Winn, Joshua N., Johnson, John Asher, Howard, Andrew W., Marcy, Geoffrey W., Isaacson, Howard, Shporer, Avi, Á. Bakos, Gáspár, Hartman, Joel D. +1 more·2010·The Astrophysical Journal

Abstract

We find the orbit of the Neptune-sized exoplanet HAT-P-11b to be highly inclined relative to the equatorial plane of its host star. This conclusion is based on spectroscopic observations of two transits, which allowed the Rossiter–McLaughlin effect to be detected with an amplitude of 1.5 m s −1 . The sky-projected obliquity is 103 +26 −10 deg. This is the smallest exoplanet for which spin–orbit alignment has been measured. The result favors a migration scenario involving few-body interactions followed by tidal dissipation. This finding also conforms with the pattern that the systems with the weakest tidal interactions have the widest spread in obliquities. We predict that the high obliquity of HAT-P-11 will be manifest in transit light curves from the Kepler spacecraft: starspot-crossing anomalies will recur at most once per stellar rotation period, rather than once per orbital period as they would for a well-aligned system.

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Crossref · 10.1088/2041-8205/723/2/l223

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  • Exoplanetary systems around sun-like stars generically exhibit a very broad range of spin-orbit misalignments, with projected stellar obliquities ranging from 0 to 180 deg.

    “Over the last decade, observations of the Rossiter-McLaughlin e ect (see for example Winn et al. 2010; Triaud 2017) and doppler tomography (e.g., Marsh 2001; Johnson et al. 2017) have revealed that exoplanetary systems around sun-like stars generically exhibit a very broad range of spinorbit misalignments, with projected stellar obliquities ranging from 0 to 180 deg.”

    From The planet nine hypothesis (2019) · cites this paper as Winn et al. 2010

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Authors
Winn, J. N., Johnson, J. A., Howard, A. W., Marcy, G. W., Isaacson, H., Shporer, A., Á. Bakos, G., Hartman, J. D., & Albrecht, S.
Affiliations
  • Massachusetts Institute of Technology (US)
  • California Institute of Technology (US)
  • Space Sciences Laboratory (US)
  • Las Cumbres Observatory Global Telescope Network (US)
  • Center for Astrophysics Harvard & Smithsonian (US)
Venue
The Astrophysical Journal
Published
2010-10-20
Volume
723
Issue
2
Pages
L223-L227
ISSN
  • 2041-8205 (ISSN-L)
  • 2041-8213
OpenAlex
W1992258122
Cited by
172
References
1
Citations by year
2026: 2 · 2025: 7 · 2024: 6 · 2023: 4 · 2022: 5 · 2021: 6 · 2020: 10 · 2019: 10 · 2018: 33 · 2017: 8 · 2016: 10 · 2015: 8 · 2014: 17 · 2013: 10 · 2012: 15
FWCI
8.22
Type
journal article
Language
en
Open access
Locations
  • The Astrophysical Journal Letters (publishedVersion)
  • arXiv (Cornell University) (submittedVersion)
  • CaltechAUTHORS (California Institute of Technology) (submittedVersion)
  • arXiv (Cornell University)
Funders
  • National Science Foundation (0702843)
  • National Aeronautics and Space Administration (NNX09AD36G, NNX08AF23G)
  • W. M. Keck Foundation
  • California Institute of Technology
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
HAT-P-11b, super-Neptune, orbital obliquity, spin-orbit misalignment, Rossiter-McLaughlin effect, exoplanet transits, tidal dissipation, planet migration, stellar rotation, transit light curves, Kepler

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