Temperate Earth-sized planets transiting a nearby ultracool dwarf star
Michael Gillon, Emmanuel Jehin, Susan M. Lederer, Laetitia Delrez,, Julien de Wit, Artem Burdanov, Valerie Van Grootel, Adam J. Burgasser, Amaury, H. M. J. Triaud, Cyrielle Opitom, Brice-Olivier Demory, Devendra K. Sahu,, Daniella Bardalez Gagliuffi, Pierre Magain, Didier Queloz

TL;DR
This paper reports the discovery of three Earth-sized planets transiting a nearby ultracool dwarf star, with two planets near the habitable zone, providing a valuable target for detailed characterization of such planetary systems.
Contribution
First detection of multiple Earth-sized planets orbiting a nearby ultracool dwarf, confirming theoretical predictions of their existence and potential habitability.
Findings
Two planets are near the habitable zone with Earth-like irradiation.
The third planet's orbit remains uncertain, possibly less irradiated than Earth.
The host star's brightness allows detailed future study of the system.
Abstract
Star-like objects with effective temperatures of less than 2,700 kelvin are referred to as ultracool dwarfs. This heterogeneous group includes stars of extremely low mass as well as brown dwarfs (substellar objects not massive enough to sustain hydrogen fusion), and represents about 15 per cent of the population of astronomical objects near the Sun. Core-accretion theory predicts that, given the small masses of these ultracool dwarfs, and the small sizes of their protoplanetary disk, there should be a large but hitherto undetected population of terrestrial planets orbiting them - ranging from metal-rich Mercury-sized planets to more hospitable volatile-rich Earth-sized planets. Here we report observations of three short-period Earth-sized planets transiting an ultracool dwarf star only 12 parsecs away. The inner two planets receive four times and two times the irradiation of Earth,…
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