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FältnamnIndikatorerMetadata
00005402naa a2200901 4500
001oai:research.chalmers.se:97fdb929-51ee-4e14-9317-9bf4a55ebe26
003SwePub
008181012s2018 | |||||||||||000 ||eng|
024a https://doi.org/10.1051/0004-6361/2018328672 DOI
024a https://research.chalmers.se/publication/5053292 URI
024a https://research.chalmers.se/publication/5057462 URI
024a https://research.chalmers.se/publication/5062922 URI
040 a (SwePub)cth
041 a engb eng
042 9 SwePub
072 7a art2 swepub-publicationtype
072 7a ref2 swepub-contenttype
100a Persson, Carina,d 1964u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)carina64
2451 0a Super-Earth of 8 Mearth in a 2.2-day orbit around the K5V star K2-216
264 c 2018-10-10
264 1b EDP Sciences,c 2018
338 a electronic2 rdacarrier
520 a Although thousands of exoplanets have been discovered to date, far fewer have been fully characterised, in particular super- Earths. The KESPRINT consortium identified K2-216 as a planetary candidate host star in the K2 space mission Campaign 8 field with a transiting super-Earth. The planet has recently been validated as well. Our aim was to confirm the detection and derive the main physical characteristics of K2-216b, including the mass. We performed a series of follow-up observations: high resolution imaging with the FastCam camera at the TCS, the Infrared Camera and Spectrograph at Subaru, and high resolution spectroscopy with HARPS (ESO, La Silla), HARPS-N (TNG), and FIES (NOT). The stellar spectra were analyzed with the SpecMatch-Emp and SME codes to derive the stellar fundamental properties. We analyzed the K2 light curve with the Pyaneti software. The radial-velocity measurements were modelled with both a Gaussian process (GP) regression and the floating chunk offset (FCO) technique to simultaneously model the planetary signal and correlated noise associated with stellar activity. Imaging confirms that K2-216 is a single star. Our analysis discloses that the star is a moderately active K5V star of mass 0.70+/-0.03 Msun and radius 0.72+/-0.03 Rsun. Planet b is found to have a radius of 1.75+0.17-0.10 Rearth and a 2.17-day orbit in agreement with previous results. We find consistent results for the planet mass from both models: 7.4+/-2.2 Mearth from the GP regression, and 8.0+/-1.6 Mearth from the FCO technique, which implies that this planet is a super-Earth. The planet parameters put planet b in the middle of, or just below, the gap of the radius distribution of small planets. The density is consistent with a rocky composition of primarily iron and magnesium silicate. In agreement with theoretical predictions, we find that the planet is a remnant core, stripped of its atmosphere, and is one of the largest planets found that has lost its atmosphere.
650 7a NATURVETENSKAPx Fysikx Astronomi, astrofysik och kosmologi0 (SwePub)103052 hsv//swe
650 7a NATURAL SCIENCESx Physical Sciencesx Astronomy, Astrophysics and Cosmology0 (SwePub)103052 hsv//eng
653 a Stars: individual: K2-216
653 a Planets and satellites: Atmospheres
653 a Techniques: photometric
653 a Techniques: radial velocities
653 a Planetary systems
653 a Planets and satellites: composition
700a Fridlund, Malcolm,d 1952u Chalmers tekniska högskola,Chalmers University of Technology4 aut0 (Swepub:cth)malfri
700a Barragan, O.4 aut
700a Dai, F.4 aut
700a Gandolfi, D.4 aut
700a Hatzes, A. P.4 aut
700a Hirano, T.4 aut
700a Grziwa, S.4 aut
700a Korth, J.4 aut
700a Prieto-Arranz, J.4 aut
700a Fossati, L.4 aut
700a Van Eylen, V.4 aut
700a Justesen, A. Bo4 aut
700a Livingston, J.4 aut
700a Kubyshkina, D.4 aut
700a Deeg, H. J.4 aut
700a Guenther, E. W.4 aut
700a Nowak, G.4 aut
700a Cabrera, J.4 aut
700a Eigmüller, Ph4 aut
700a Csizmadia, Sz.4 aut
700a Smith, A. M. S.4 aut
700a Erikson, A.4 aut
700a Albrecht, S.4 aut
700a Alonso, R.4 aut
700a Cochran, W. D.4 aut
700a Endl, M.4 aut
700a Esposito, M.4 aut
700a Fukui, A.4 aut
700a Heeren, P.4 aut
700a Hidalgo, D.4 aut
700a Hjorth, M.4 aut
700a Kuzuhara, M.4 aut
700a Narita, N.4 aut
700a Nespral, D.4 aut
700a Palle, E.4 aut
700a Pätzold, M.4 aut
700a Rauer, H.4 aut
700a Rodler, F.4 aut
700a Winn, J. N.4 aut
710a Chalmers tekniska högskola4 org
773t Astronomy and Astrophysicsd : EDP Sciencesg 618:33q 618:33x 0004-6361x 1432-0746
856u https://research.chalmers.se/publication/506292/file/506292_Fulltext.pdfx primaryx freey FULLTEXT
856u https://www.aanda.org/articles/aa/pdf/2018/10/aa32867-18.pdf
8564 8u https://doi.org/10.1051/0004-6361/201832867
8564 8u https://research.chalmers.se/publication/505329
8564 8u https://research.chalmers.se/publication/505746
8564 8u https://research.chalmers.se/publication/506292

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