description Kepler-444 e Overview
Kepler-444 e is a confirmed sub-Earth exoplanet in the Kepler-444 system, which orbits a metal-poor K-type star in the Milky Way. The host star is estimated to be about 11 billion years old, making this a compact planetary system formed early in the history of the Galaxy. The planet is relevant to studies of small planets around old stars and to comparisons between ancient planetary systems and the Solar System.
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