K2-140b - an eccentric 6.57 d transiting hot Jupiter in Virgo
Abstract
We present the discovery of K2-140b, a P = 6.57 d Jupiter-mass (MP = 1.019 ± 0.070MJup) planet transiting a V = 12.5 (G5-spectral type) star in an eccentric orbit (e = 0.120^{+0.056}_{-0.046}) detected using a combination of K2 photometry and ground-based observations. With a radius of 1.095 ± 0.018 RJup, the planet has a bulk density of 0.726 ± 0.062 ρJup. The host star has a [Fe/H] of 0.12 ± 0.045, and from the K2 light curve, we find a rotation period for the star of 16.3 ± 0.1 d. This discovery is the 9th hot Jupiter from K2 and highlights K2's ability to detect transiting giant planets at periods slightly longer than traditional, ground-based surveys. This planet is slightly inflated, but much less than others with similar incident fluxes. These are of interest for investigating the inflation mechanism of hot Jupiters.
- Publication:
-
Monthly Notices of the Royal Astronomical Society
- Pub Date:
- April 2018
- DOI:
- arXiv:
- arXiv:1706.06865
- Bibcode:
- 2018MNRAS.475.1809G
- Keywords:
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- techniques: high angular resolution;
- techniques: photometric;
- techniques: radial velocities;
- planets and satellites: detection;
- stars: individual: K2-140;
- Astrophysics - Earth and Planetary Astrophysics
- E-Print:
- Submitted to MNRAS, 11 pages, 10 figures