An ancient extrasolar system with five sub-Earth-size planets
T. L. Campante, T. Barclay, J. J. Swift, D. Huber, V. Zh. Adibekyan,, W. Cochran, C. J. Burke, H. Isaacson, E. V. Quintana, G. R. Davies, V. Silva, Aguirre, D. Ragozzine, R. Riddle, C. Baranec, S. Basu, W. J. Chaplin, J., Christensen-Dalsgaard, T. S. Metcalfe, T. R. Bedding

TL;DR
This paper reports the discovery and detailed characterization of Kepler-444, an ancient star hosting five small, terrestrial-sized planets, demonstrating that Earth-sized planets formed early in the Universe's history over 11 billion years ago.
Contribution
It provides the first precise age measurement of an old star hosting multiple terrestrial planets, showing such planets existed early in cosmic history.
Findings
Kepler-444 is approximately 11.2 billion years old.
The system hosts five planets smaller than Earth.
Earth-sized planets formed over 11 billion years ago.
Abstract
The chemical composition of stars hosting small exoplanets (with radii less than four Earth radii) appears to be more diverse than that of gas-giant hosts, which tend to be metal-rich. This implies that small, including Earth-size, planets may have readily formed at earlier epochs in the Universe's history when metals were more scarce. We report Kepler spacecraft observations of Kepler-444, a metal-poor Sun-like star from the old population of the Galactic thick disk and the host to a compact system of five transiting planets with sizes between those of Mercury and Venus. We validate this system as a true five-planet system orbiting the target star and provide a detailed characterization of its planetary and orbital parameters based on an analysis of the transit photometry. Kepler-444 is the densest star with detected solar-like oscillations. We use asteroseismology to directly measure…
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