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dc.contributor.authorJohnson, John Asher
dc.contributor.authorWinn, Joshua Nathan
dc.contributor.authorAlbrecht, Simon H.
dc.contributor.authorHoward, Andrew W.
dc.contributor.authorMarcy, Geoffrey W.
dc.contributor.authorGazak, J. Zachary
dc.date.accessioned2013-02-14T20:18:10Z
dc.date.available2013-02-14T20:18:10Z
dc.date.issued2009-09
dc.date.submitted2009-07
dc.identifier.issn0004-6280
dc.identifier.issn1538-3873
dc.identifier.urihttp://hdl.handle.net/1721.1/77088
dc.description.abstractWe presented evidence that the WASP-14 exoplanetary system has misaligned orbital and stellar-rotational axes, with an angle of 33.1 plus or minus 7.4 degrees between their sky projections. At the time of this publication, WASP-14 was the third system known to have a significant spin-orbit misalignment, and all three systems had super- Jupiter planets and eccentric orbits. Therefore we hypothesized that the migration and subsequent orbital evolution of massive, eccentric exoplanets is somehow different from that of less massive close-in Jupiters, the majority of which have well-aligned orbits.en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (NASA Origins of Solar Systems program, award NNX09AD36G)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (NASA Origins of Solar Systems program, award NNX09AB33G)en_US
dc.description.sponsorshipNational Science Foundation (U.S.) (NSF Astronomy and Astrophysics Postdoctoral Fellow, grant AST-0702821)en_US
dc.description.sponsorshipMassachusetts Institute of Technology (Class of 1942)en_US
dc.description.sponsorshipNetherlands Organization for Scientific Research (Rubicon fellowship)en_US
dc.description.sponsorshipUnited States. National Aeronautics and Space Administration (NASA grant NNG05GK92G)en_US
dc.description.sponsorshipUniversity of California, Berkeley (Space Sciences Laboratory,Townes Postdoctoral Fellowship)en_US
dc.language.isoen_US
dc.publisherUniversity of Chicago Pressen_US
dc.rightsCreative Commons Attribution-Noncommercial-Share Alike 3.0en_US
dc.rights.urihttp://creativecommons.org/licenses/by-nc-sa/3.0/en_US
dc.sourcearXiven_US
dc.titleA Third Exoplanetary System with Misaligned Orbital and Stellar Spin Axesen_US
dc.typeArticleen_US
dc.identifier.citationJohnson, John Asher et al. “A Third Exoplanetary System with Misaligned Orbital and Stellar Spin Axes1.” Publications of the Astronomical Society of the Pacific 121.884 (2009): 1104–1111. Web. DOI:10.1086/644604.en_US
dc.contributor.departmentMassachusetts Institute of Technology. Department of Physicsen_US
dc.contributor.departmentMIT Kavli Institute for Astrophysics and Space Researchen_US
dc.contributor.mitauthorWinn, Joshua Nathan
dc.contributor.mitauthorAlbrecht, Simon H.
dc.relation.journalPublications of the Astronomical Society of the Pacificen_US
dc.eprint.versionAuthor's final manuscripten_US
dc.type.urihttp://purl.org/eprint/type/JournalArticleen_US
eprint.statushttp://purl.org/eprint/status/PeerRevieweden_US
dspace.orderedauthorsJohnson, John A.; Winn, Joshua N.; Albrecht, Simon; Howard, Andrew W.; Marcy, Geoffrey W.; Gazak, J. Zacharyen_US
dc.identifier.orcidhttps://orcid.org/0000-0002-4265-047X
mit.licenseOPEN_ACCESS_POLICYen_US
mit.metadata.statusComplete


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