Kepler-442

Kepler-442b (also known by its Kepler object of interest designation KOI-4742.01) is a confirmed near-Earth-sized exoplanet, likely rocky, orbiting within the habitable zone of the K-type main-sequence star Kepler-442, about from Earth in the constellation of Lyra.

= 7.73, and the Sun, \scriptstyle M_{V_{\odot = 4.83, the visual luminosity of Kepler-442 is calculated from: \scriptstyle \frac{L_{V_{\ast}{L_{V_{\odot} = 10^{0.4\left(M_{V_{\odot - M_{V_{\ast\right)} | age_gyr =