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WASP-17b: AN ULTRA-LOW DENSITY PLANET IN A PROBABLE RETROGRADE ORBIT
Open accessAbstract
We report the discovery of the transiting giant planet WASP-17b, the least-dense planet currently known. It is 1.6 Saturn masses, but 1.5–2 Jupiter radii, giving a density of 6%–14% that of Jupiter. WASP-17b is in a 3.7 day orbit around a sub-solar metallicity, V = 11.6, F6 star. Preliminary detection of the Rossiter–McLaughlin effect suggests that WASP-17b is in a retrograde orbit (λ ≈ −150°), indicative of a violent history involving planet–planet or star–planet scattering. WASP-17b's bloated radius could be due to tidal heating resulting from recent or ongoing tidal circularization of an eccentric orbit, such as the highly eccentric orbits that typically result from scattering interactions. It will thus be important to determine more precisely the current orbital eccentricity by further high-precision radial velocity measurements or by timing the secondary eclipse, both to reduce the uncertainty on the planet's radius and to test tidal-heating models. Owing to its low surface gravity, WASP-17b's atmosphere has the largest scale height of any known planet, making it a good target for transmission spectroscopy.
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“Extrasolar planets have been detected with their orbital axes inclined by more than 90 degrees with respect to their star's rotation axis (e.g.WASP-17b; Anderson et al. 2010).”
From Constraints on the size and dynamics of the J1407b ring system (2016) · cites this paper as Anderson et al. 2010
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Jordi, C., Høg, E., Brown, A. G. A., Lindegren, L., Bailer‐Jones, C. A. L., Carrasco, J. M., Knude, J., Straižys, V., de Bruijne, J. H. J., Claeskens, J.-F., et al. (2006) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2005.09944.x · Cited by 49
Winn, J. N., Holman, M. J., Carter, J. A., Torres, G., Osip, D. J., & Beatty, T. G. (2012) · Cited by 45
The Transit Light Curve Project. X. A Christmas Transit of HD 17156bPreprint
Winn, J. N., Holman, M. J., Henry, G. W., Torres, G., Fischer, D. A., Johnson, J. A., Marcy, G. W., Shporer, A., & Mazeh, T. (2012) · Cited by 33
Rotation and Lithium Surface Abundances, Revisited
Böhm‐Vitense, E. (2004) · The Astronomical Journal · doi:10.1086/425053 · Cited by 24
On the Track of Very Low-mass Planets with HARPS
Pepe, F. A., Mayor, M., Queloz, D. P., Benz, W., Bertaux, J., Bouchy, F., Lovis, C., Mordasini, C., Santos, N. C., Sivan, J. P., et al. (2005) · The Messenger · Cited by 23
Self-citationSpin-orbit misalignement for the transiting planet HD 80606bPreprint
Gillon, M. (2009) · arXiv (Cornell University) · doi:10.48550/arxiv.0906.4904 · Cited by 7
Self-citation
Research works printed but not linked: 4
- Mayor, 2003, Messenger, 114, 20
- Pepe, 2005, Messenger, 120, 22
- Queloz, 2000, A&A, 359, L13
- Queloz, 2000, A&A, 354, 99
Cited by
Sorted by citations
HOT STARS WITH HOT JUPITERS HAVE HIGH OBLIQUITIES
Winn, J. N., Fabrycky, D., Albrecht, S., & Johnson, J. A. (2010) · The Astrophysical Journal · doi:10.1088/2041-8205/718/2/l145 · Cited by 735
Southworth, J. H. (2011) · Monthly Notices of the Royal Astronomical Society · doi:10.1111/j.1365-2966.2011.19399.x · Cited by 560
Spin-orbit angle measurements for six southern transiting planets
Triaud, A. H. M. J., Cameron, A. C., Queloz, D. P., Anderson, D. R., Gillon, M., Hebb, L., Hellier, C., Loeillet, B., Maxted, P. F. L., Mayor, M., et al. (2010) · Astronomy and Astrophysics · doi:10.1051/0004-6361/201014525 · Cited by 481
Self-citationKnutson, H. A., Fulton, B. J., Montet, B. T., Kao, M., Ngo, H., Howard, A. W., Crepp, J. R., Hinkley, S., Bakos, G. Á., Batygin, K., et al. (2014) · The Astrophysical Journal · doi:10.1088/0004-637x/785/2/126 · Cited by 353
IMPROVED SPECTROSCOPIC PARAMETERS FOR TRANSITING PLANET HOSTS
Torres, G., Fischer, D. A., Sozzetti, A., Buchhave, L. A., Winn, J. N., Holman, M. J., & Carter, J. A. (2012) · The Astrophysical Journal · doi:10.1088/0004-637x/757/2/161 · Cited by 326
Metadata
- Authors
- 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., Bentley, S. J., Enoch, B., Horne, K., Lister, T. A., Mayor, M., Parley, N. R., Pepe, F., Pollacco, D., Ségransan, D., Udry, S., & Wilson, D. M.
- Affiliations
- Keele University (GB)
- University of Geneva (CH)
- University of St Andrews (GB)
- University of Leicester (GB)
- Las Cumbres Observatory Global Telescope Network (US)
- Queen's University Belfast (GB)
- University of Kent (GB)
- ORCID
- Venue
- The Astrophysical Journal
- Publisher
- American Astronomical Society
- Published
- 2009-12-29
- Volume
- 709
- Issue
- 1
- Pages
- 159-167
- ISSN
- 0004-637X (ISSN-L)
- 1538-4357
- OpenAlex
- W2137800231
- Cited by
- 208
- References
- 89
- Citations by year
- 2026: 5 · 2025: 5 · 2024: 6 · 2023: 8 · 2022: 10 · 2021: 1 · 2020: 3 · 2019: 6 · 2018: 9 · 2017: 8 · 2016: 15 · 2015: 6 · 2014: 4 · 2013: 12 · 2012: 27
- FWCI
- 18.46
- Type
- journal article
- Language
- en
- Open access
- bronze
- doi.org
- Locations
- The Astrophysical Journal (publishedVersion)
- University of Birmingham Research Portal (University of Birmingham) (publishedVersion)
- arXiv (Cornell University) (submittedVersion)
- ORBi (University of Liège) (submittedVersion, other-oa)
- Leicester Research Archive (University of Leicester) (submittedVersion)
- Research Portal (Queen's University Belfast) (submittedVersion)
- arXiv (Cornell University)
- Funders
- Queen's University Belfast
- Queen's University
- Science and Technology Facilities Council (PP/F000081/1, ST/I002308/1, PP/F000065/1, PP/F000057/1, PP/F000073/1, PP/D000955/1, ST/G002355/1, ST/G001987/1)
- 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 › Instrumentation › Astronomy and Astrophysical Research
- Keywords
- WASP-17b, transiting exoplanets, retrograde orbits, Rossiter-McLaughlin effect, planet-planet scattering, tidal heating, orbital eccentricity, tidal circularization, transmission spectroscopy, atmospheric scale height, low surface gravity, hot Jupiters
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
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