Projects per year
Abstract
We present the confirmation of a small, moderately-irradiated (F= 155±7 F⊕) Neptune with a substantial gas envelope in a P=11.8728787±0.0000085-day orbit about a quiet, Sun-like G0V star Kepler-1655. Based on our analysis of the Kepler light curve, we determined Kepler-1655b’s radius to be 2.213±0.082 R⊕. We acquired 95 high-resolution spectra with TNG/HARPS-N, enabling us to characterize the host star and determine an accurate mass for Kepler-1655b of 5.0±^3.1_2.8 M⊕ via Gaussian-process regression. Our mass determination excludes an Earth-like composition with 98% confidence. Kepler-1655b falls on the upper edge of the evaporation valley, in the relatively sparsely occupied transition region between rocky and gas-rich planets. It is therefore part of a population of planets that we should actively seek to characterize further.
| Original language | English |
|---|---|
| Article number | 203 |
| Number of pages | 19 |
| Journal | Astronomical Journal |
| Volume | 155 |
| Issue number | 5 |
| Early online date | 20 Apr 2018 |
| DOIs | |
| Publication status | Published - May 2018 |
Keywords
- Planets and satellites: detection
- Planets and satellites: gaseous planets
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Dive into the research topics of 'An accurate mass determination for Kepler-1655b, a moderately-irradiated world with a significant volatile envelope'. Together they form a unique fingerprint.Projects
- 2 Finished
-
Astronomy at St Andrews 2015-2018: Astronomy at St Andrews 2015-2018
Jardine, M. (PI), Cameron, A. (CoI), Cyganowski, C. (CoI), Horne, K. (CoI) & Wood, K. (CoI)
Science & Technology Facilities Council
1/04/15 → 31/03/18
Project: Standard
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EU FP7 Space ETAEARTH: ETAEARTH
Cameron, A. (PI)
Joint Research Centre European Commission
1/01/13 → 31/12/17
Project: Standard
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