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dc.contributor.authorAnglada-Escude, Guillem
dc.contributor.authorArriagada, P.
dc.contributor.authorTuomi, Mikko
dc.contributor.authorZechmeister, M.
dc.contributor.authorJenkins, J. S.
dc.contributor.authorOfir, A.
dc.contributor.authorDreizler, S.
dc.contributor.authorGerlach, E.
dc.contributor.authorMarvin, C. J.
dc.contributor.authorReiners, A.
dc.contributor.authorJeffers, S. V.
dc.contributor.authorButler, R.P.
dc.contributor.authorVogt, S. S.
dc.contributor.authorAmado, P. J.
dc.contributor.authorGerlach, E.
dc.contributor.authorRodríguez-López, C.
dc.contributor.authorBerdiñas, Z. M.
dc.contributor.authorMorin, J.
dc.contributor.authorCrane, J. D.
dc.contributor.authorShectman, S. A.
dc.contributor.authorThompson, Ian B.
dc.contributor.authorDiaz, M.
dc.contributor.authorRivera, E.
dc.contributor.authorSarmiento, L. F.
dc.contributor.authorJones, Hugh
dc.date.accessioned2017-08-11T14:59:48Z
dc.date.available2017-08-11T14:59:48Z
dc.date.issued2014-09-01
dc.identifier.citationAnglada-Escude , G , Arriagada , P , Tuomi , M , Zechmeister , M , Jenkins , J S , Ofir , A , Dreizler , S , Gerlach , E , Marvin , C J , Reiners , A , Jeffers , S V , Butler , R P , Vogt , S S , Amado , P J , Gerlach , E , Rodríguez-López , C , Berdiñas , Z M , Morin , J , Crane , J D , Shectman , S A , Thompson , I B , Diaz , M , Rivera , E , Sarmiento , L F & Jones , H 2014 , ' Two planets around Kapteyn's star: a cold and a temperate super-Earth orbiting the nearest halo red dwarf ' , Monthly Notices of the Royal Astronomical Society , vol. 443 , no. 1 , pp. L89-L93 . https://doi.org/10.1093/mnrasl/slu076
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 10455570
dc.identifier.otherPURE UUID: 0b7a3d32-c18d-408c-8672-ad66e37fdc08
dc.identifier.otherScopus: 84905192298
dc.identifier.urihttp://hdl.handle.net/2299/19219
dc.descriptionThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society - Letters. ©: 2014 The Author(s). Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved.
dc.description.abstractExoplanets of a few Earth masses can be now detected around nearby low-mass stars using Doppler spectroscopy. In this Letter, we investigate the radial velocity variations of Kapteyn's star, which is both a sub-dwarf M-star and the nearest halo object to the Sun. The observations comprise archival and new HARPS (High Accuracy Radial velocity Planet Searcher), High Resolution Echelle Spectrometer (HIRES) and Planet Finder Spectrograph (PFS) Doppler measurements. Two Doppler signals are detected at periods of 48 and 120 d using likelihood periodograms and a Bayesian analysis of the data. Using the same techniques, the activity indices and archival All Sky Automated Survey (ASAS-3) photometry show evidence for low-level activity periodicities of the order of several hundred days. However, there are no significant correlations with the radial velocity variations on the same time-scales. The inclusion of planetary Keplerian signals in the model results in levels of correlated and excess white noise that are remarkably low compared to younger G, K and M dwarfs. We conclude that Kapteyn's star is most probably orbited by two super-Earth mass planets, one of which is orbiting in its circumstellar habitable zone, becoming the oldest potentially habitable planet known to date. The presence and long-term survival of a planetary system seem a remarkable feat given the peculiar origin and kinematic history of Kapteyn's star. The detection of super-Earth mass planets around halo stars provides important insights into planet-formation processes in the early days of the Milky Way.en
dc.format.extent5
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleTwo planets around Kapteyn's star: a cold and a temperate super-Earth orbiting the nearest halo red dwarfen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionVoR
rioxxterms.versionofrecordhttps://doi.org/10.1093/mnrasl/slu076
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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