Kepler's found some 2,000
+ planets orbiting stars and published its data to allow citizen scientists to confirm their findings.
Not exact matches
Planet b has a close inner
orbit around
Star A at a semi-major axis of only 0.0717
+ / - 0.0034 AUs (Howard et al, 2014).
Astronomers have also observed that
planet b is eclipsed by its
star by about two minutes (120
+ / - 24 seconds) later than would be expected if it has a perfectly circular
orbit.
The inner
planet, Kepler - 69b, has a radius of 2.24
+ / -0.4 Rearth and
orbits the host
star every 13.7 days.
We designate the
planet TrES - 1; its inferred mass is 0.75
+... ▽ More We report the detection of a transiting Jupiter - sized
planet orbiting a relatively bright (V = 11.79) K0V
star.
The characteristics of the host
star are well constrained by high - resolution spectroscopy combined with an asteroseismic analysis of the Kepler photometry, leading to an estimated mass and radius of 0.970
+ / - 0.060 M... ▽ More A search of the time - series photometry from NASA's Kepler spacecraft reveals a transiting
planet candidate
orbiting the 11th magnitude G5 dwarf KIC 10593626 with a period of 290 days.
Designated MOA -2009-BLG-266L b, the
planet has a mass of around 10.4
+ / - 1.7 Earth - masses and
orbits its host
star at a semi-major axis of 3.2
+1.9 / -0.5 AUs with an orbital period of 7.6
+7.7 / -1.5 years.
Planet b's
orbit around
Star A has a semi-major axis of only 0.0717
+ / - 0.0034 AUs (Howard et al, 2014).