Planetary Candidates Observed by Kepler.
Not exact matches
But other observations need to confirm the true
planetary nature of these
candidate events, because the
observed dips may also be due to an eclipsing binary star in the background whose light blends with the foreground star studied by Kepler.
Characterizing K2
Candidate Planetary Systems Orbiting Low - Mass Stars I: Classifying Low - mass Host Stars
Observed During Campaigns 1 - 7
Since a planet's radius and equilibrium temperature depends on the parameters of its host star, our study provides more precise
planetary parameters for planets and
candidates orbiting late - type stars
observed with K2.
The 16
planetary candidates have estimated diameters within range of being super-Earths (1.26 to 2.0 times Earth's diameter), given error margins ranging from 25 to 35 percent due to the uncertainty in the size of their host star and of the «depth» of the
observed transits (decrease in stellar luminosity) across the surface of the star.