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 K7 V 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⊕ and radius of 1.54-0.09+0.10 R⊕, 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 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.

K2-141 b: A 5- M ⊗ super-Earth transiting a K7 v star every 6.7 h

Barragán, O.;Gandolfi, D.;Antoniciello, G.;
2018-01-01

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 K7 V 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⊕ and radius of 1.54-0.09+0.10 R⊕, 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 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.
2018
612
1
11
https://www.aanda.org/
http://adsabs.harvard.edu/abs/2018A%26A...612A..95B
Planetary systems; Planets and satellites: individual: EPIC 246393474 b; Stars: fundamental parameters; Stars: individual: EPIC 246393474; Techniques: photometric; Techniques: radial velocities; Astronomy and Astrophysics; Space and Planetary Science
Barragán, 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.; Bo Justesen, A.; 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.
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Utilizza questo identificativo per citare o creare un link a questo documento: https://hdl.handle.net/2318/1693367
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