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Kepler-25

Yellow-white hued star in the constellation Lyra From Wikipedia, the free encyclopedia

Kepler-25
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Kepler-25 is a star in the northern constellation of Lyra.[1] It is slightly larger and more massive than the Sun, with a luminosity 212 times that of the Sun.[5] With an apparent visual magnitude of 10.6,[3] this star is too faint to be seen with the naked eye.

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Quick Facts Observation data Epoch J2000 Equinox J2000, Constellation ...
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Planetary system

In 2011, two candidate planets were found transiting this star by the Kepler space telescope.[10] These planets are very close to yet not lie in the 1:2 orbital resonance to each other, indicating the absence of other planetary objects in the inner part of the planetary systems.[11] These planets were confirmed through transit-timing variation method.[12] A third planet was discovered through follow-up radial velocity measurements and was confirmed in January 2014.[8]

The plane of planetary orbits is well aligned with the equatorial plane of the star, misalignment angle equal to 7±8°[13]

More information Companion (in order from star), Mass ...
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References

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