Authors:Barragán et alAbstract:We report the discovery of K2-98 b (EPIC 211391664 b), a transiting Neptune-sized planet monitored by the K2 mission during its campaign 5. We combine the K2 time-series data with ground-based photometric and spectroscopic follow-up observations to confirm the planetary nature of the object and derive its mass, radius, and orbital parameters. K2-98 b is a warm Neptune-like planet in a 10-day orbit around a V=12.2~mag F-type star with M⋆=1.074±0.042, R⋆=1.311+0.083−0.048, and age of 5.2+1.2−1.0~Gyr. We derive a planetary mass and radius of Mp=32.2±8.1 and Rp=4.3+0.3−0.2. K2-98 b joins the relatively small group of Neptune-sized planets whose both mass and radius have been derived with a precision better than 25 %. We estimate that the planet will be engulfed by its host star in ∼3~Gyr, due to the evolution of the latter towards the red giant branch.
Showing posts with label EPIC 211391664b. Show all posts
Showing posts with label EPIC 211391664b. Show all posts
Thursday, January 12, 2017
K2-98 b: A 32 Earth Mass Neptune-sized Exoplanet in a 10-day orbit around an F8 star
Labels:
engulfment,
EPIC 211391664b,
F dwarf exoplanets,
gas giants,
giant planets,
hot neptunes,
K2-98b
Thursday, December 8, 2016
EPIC 211391664b: A 32-M⊕ Neptune-sized planet in a 10-day orbit around an F8 star
Authors:Barragán et alAbstract:We report the discovery of EPIC 211391664b, a transiting Neptune-sized planet monitored by the K2 mission during its campaign 5. We combine the K2 time-series data with ground-based photometric and spectroscopic follow-up observations to confirm the planetary nature of the object and derive its mass, radius, and orbital parameters. EPIC 211391664 b is a warm Neptune-like planet in a 10-day orbit around a V=12.2~mag F-type star with M⋆=1.074±0.042M⊙, R⋆=1.311+0.083−0.048R⊙, and age of 5.2+1.2−1.0~Gyr. We derive a planetary mass and radius of Mp=32.2±8.1M⊕ and Rp=4.3+0.3−0.2R⊕. EPIC 211391664b joins the relatively small group of Neptune-sized planets whose mass and radius have been derived with a precision better than 3-σ. We estimate that the planet will be engulfed by EPIC 211391664 in ∼3~Gyr, due to the evolution of the host star towards the red giant branch.
Labels:
EPIC 211391664b,
F dwarf exoplanets,
hot neptunes,
k2 mission,
kepler
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