Barragan, O., Gandolfi, D., Smith, A. M. S., Deeg, H. J., Fridlund, M. C. V., Persson, C. M., Donati, P., Endl, M., Csizmadia, Sz., Grziwa, S., Nespral, D., Hatzes, A. P., Cochran, W. D., Fossati, L., Brems, S. S., Cabrera, J., Cusano, F., Eigmuller, Ph., Eiroa, C., Erikson, A., Guenther, E., Korth, J., Lorenzo-Oliveira, D., Mancini, L., Paetzold, M., Prieto-Arranz, J., Rauer, H., Rebollido, I., Saario, J. and Zakhozhay, O. V. (2018). K2-139 b: a low-mass warm Jupiter on a 29-d orbit transiting an active K0 V star. Mon. Not. Roy. Astron. Soc., 475 (2). S. 1765 - 1777. OXFORD: OXFORD UNIV PRESS. ISSN 1365-2966

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Abstract

We announce the discovery of K2-139 b (EPIC 218916923 b), a transiting warm- Jupiter (T-eq = 547 +/- 25 K) on a 29-d orbit around an active (log R'(HK)= -4.46 +/- 0.06) K0V star in K2 Campaign 7. We derive the system's parameters by combining the K2 photometry with ground-based follow-up observations. With a mass of 0.387(-0.075)(+0.083) M-J and radius of 0.808(-0.033)(+0.034) R-J, K2-139 b is one of the transiting warm Jupiters with the lowest mass known to date. The planetary mean density of 0.91(-0.20)(+0.24) g cm(-3) can be explained with a core of similar to 50M circle dot. Given the brightness of the host star (V = 11.653 mag), the relatively short transit duration (similar to 5 h), and the expected amplitude of the Rossiter-McLaughlin effect (similar to 25m s(-1)), K2-139 is an ideal target to measure the spin-orbit angle of a planetary system hosting a warm Jupiter.

Item Type: Journal Article
Creators:
CreatorsEmailORCIDORCID Put Code
Barragan, O.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Gandolfi, D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Smith, A. M. S.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Deeg, H. J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Fridlund, M. C. V.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Persson, C. M.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Donati, P.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Endl, M.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Csizmadia, Sz.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Grziwa, S.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Nespral, D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Hatzes, A. P.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Cochran, W. D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Fossati, L.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Brems, S. S.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Cabrera, J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Cusano, F.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Eigmuller, Ph.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Eiroa, C.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Erikson, A.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Guenther, E.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Korth, J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Lorenzo-Oliveira, D.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Mancini, L.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Paetzold, M.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Prieto-Arranz, J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Rauer, H.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Rebollido, I.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Saario, J.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
Zakhozhay, O. V.UNSPECIFIEDUNSPECIFIEDUNSPECIFIED
URN: urn:nbn:de:hbz:38-192116
DOI: 10.1093/mnras/stx3207
Journal or Publication Title: Mon. Not. Roy. Astron. Soc.
Volume: 475
Number: 2
Page Range: S. 1765 - 1777
Date: 2018
Publisher: OXFORD UNIV PRESS
Place of Publication: OXFORD
ISSN: 1365-2966
Language: English
Faculty: Unspecified
Divisions: Unspecified
Subjects: no entry
Uncontrolled Keywords:
KeywordsLanguage
LIGHT CURVES; COOL STARS; ECCENTRIC ORBIT; PLANET; EXOPLANETS; SEARCH; ATMOSPHERES; TELESCOPE; EVOLUTION; SPECTRAMultiple languages
Astronomy & AstrophysicsMultiple languages
Refereed: Yes
URI: http://kups.ub.uni-koeln.de/id/eprint/19211

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