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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 ± 0.018RJup, the planet has a bulk density of 0.726 ± 0.062ρJup. 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 ± 0.1d. 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.
Original language | English |
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Pages (from-to) | 1809-1818 |
Journal | Monthly Notices of the Royal Astronomical Society |
Volume | 475 |
Issue number | 2 |
Early online date | 5 Jan 2018 |
DOIs | |
Publication status | Published - 1 Apr 2018 |
Keywords
- Techniques: high angular resolution
- Techniques: photometric
- Techniques: radial velocities
- Planets and satellites: detection
- Stars: individual: K2-140
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Dive into the research topics of 'K2-140b - an eccentric 6.57 d transiting hot Jupiter in Virgo'. Together they form a unique fingerprint.Projects
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Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018
Jardine, M. M. (PI), Cameron, A. C. (CoI), Cyganowski, C. J. (CoI), Horne, K. D. (CoI) & Wood, K. (CoI)
Science & Technology Facilities Council
1/04/15 → 31/03/18
Project: Standard