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K2-141 b A 5-M-circle plus super-Earth transiting a K7V star every 6.7 h

Authors :
Barragan, O.
Gandolfi, D.
Dai, F.
Livingston, J.
Persson, C. M.
Hirano, T.
Narita, N.
Csizmadia, Sz.
Winn, J. N.
Nespral, D.
Prieto-Arranz, J.
Smith, A. M. S.
Nowak, G.
Albrecht, S.
Antoniciello, G.
Justesen, A. Bo
Cabrera, J.
Cochran, W. D.
Deeg, H.
Eigmuller, Ph.
Endl, M.
Erikson, A.
Fridlund, M.
Fukui, A.
Grziwa, S.
Guenther, E.
Hatzes, A. P.
Hidalgo, D.
Johnson, M. C.
Korth, J.
Palle, E.
Patzold, M.
Rauer, H.
Tanaka, Y.
Van Eylen, V.
Barragan, O.
Gandolfi, D.
Dai, F.
Livingston, J.
Persson, C. M.
Hirano, T.
Narita, N.
Csizmadia, Sz.
Winn, J. N.
Nespral, D.
Prieto-Arranz, J.
Smith, A. M. S.
Nowak, G.
Albrecht, S.
Antoniciello, G.
Justesen, A. Bo
Cabrera, J.
Cochran, W. D.
Deeg, H.
Eigmuller, Ph.
Endl, M.
Erikson, A.
Fridlund, M.
Fukui, A.
Grziwa, S.
Guenther, E.
Hatzes, A. P.
Hidalgo, D.
Johnson, M. C.
Korth, J.
Palle, E.
Patzold, M.
Rauer, H.
Tanaka, Y.
Van Eylen, V.
Publication Year :
2018

Abstract

We report on the discovery of K2-141 b (EPIC 246393474 b), an ultra-short-period super-Earth on a 6.7 h orbit transiting an active K7V star based on data from K2 campaign 12. We confirmed the planet's existence and measured its mass with a series of follow-up observations: seeing-limited MuSCAT imaging, NESSI high-resolution speckle observations, and FIES and HARPS high-precision radial-velocity monitoring. K2-141 b has a mass of 5.31 +/- 0.46 M-circle plus and radius of 1.54(-0.09)(+0.10), yielding a mean density of 8.00(-1.45)(+1.83) g cm(-3) and suggesting a rocky-iron composition. Models indicate that iron cannot exceed similar to 70% of the total mass. With an orbital period of only 6.7 h, K2-141 b is the shortest-period planet known to date with a precisely determined mass.

Details

Database :
OAIster
Notes :
English
Publication Type :
Electronic Resource
Accession number :
edsoai.on1201319355
Document Type :
Electronic Resource