
Judith Korth
Postdoc

K2-290 : A warm Jupiter and a mini-Neptune in a triple-star system
Author
Summary, in English
We report the discovery of two transiting planets orbiting K2-290 (EPIC 249624646), a bright (V = 11.11) late F-type star residing in a triple-star system. It was observed during Campaign 15 of the K2 mission, and in order to confirm and characterize the system, follow-up spectroscopy and AO imaging were carried out using the FIES, HARPS, HARPS-N, and IRCS instruments. From AO imaging and Gaia data we identify two M-dwarf companions at a separation of 113 ± 2 and 2467+−177155 au. From radial velocities, K2 photometry, and stellar characterization of the host star, we find the inner planet to be a mini-Neptune with a radius of 3.06 ± 0.16 R and an orbital period of P = 9.2 d. The radius of the mini-Neptune suggests that the planet is located above the radius valley, and with an incident flux of F ∼ 400 F, it lies safely outside the super-Earth desert. The outer warm Jupiter has a mass of 0.774 ± 0.047 MJ and a radius of 1.006 ± 0.050 RJ, and orbits the host star every 48.4 d on an orbit with an eccentricity e < 0.241. Its mild eccentricity and mini-Neptune sibling suggest that the warm Jupiter originates from in situ formation or disc migration.
Publishing year
2019-04-11
Language
English
Pages
3522-3536
Publication/Series
Monthly Notices of the Royal Astronomical Society
Volume
484
Issue
3
Document type
Journal article
Publisher
Oxford University Press
Keywords
- Planets
- Planets and satellites: detection
- Planets and satellites: formation
- Planets and satellites: individual: K2-290
- Satellites: individual: EPIC 249624646
Status
Published
ISBN/ISSN/Other
- ISSN: 0035-8711