Today’s authors carefully check their evidence for the first potential exomoon detection.
Using new Gaia data, the authors update the stellar radii for the majority of Kepler’s stars. While they find that most stars have similar radii to previous reported values, there are some large discrepancies.
In today’s paper, after years spent on an impasse, we finally arrive at a consensus on the mass of the rocky exoplanet Kepler-10c. The discussion yields many important lessons on how to properly analyze radial velocities.
Why can’t more exoplanet systems be like TRAPPIST-1? Why do so many Kepler systems have only one transiting planet? Today’s paper tries to answer both questions.
The Kepler-11 system features 5 planets packed within the orbit of Mercury. Read on to hear about their discovery, analysis, and what this system says about planetary migration.