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π Earth: A 3.14 day Earth-sized Planet from K2's Kitchen Served Warm by the SPECULOOS Team

Author(s)
Niraula, Prajwal; de Wit, Julien; Rackham, Benjamin V; Ducrot, Elsa; Burdanov, Artem; Crossfield, Ian J. M.; Grootel, Valérie Van; Murray, Catriona; Garcia, Lionel J.; Alonso, Roi; Beard, Corey; Maqueo Chew, Yilen Gómez; Delrez, Laetitia; Demory, Brice-Olivier; Fulton, Benjamin J.; Gillon, Michaël; Günther, Maximilian N.; Howard, Andrew W.; Issacson, Howard; Jehin, Emmanuël; Pedersen, Peter P.; Pozuelos, Francisco J.; Queloz, Didier; Rebolo-López, Rafael; Lalitha, Sairam; Sebastian, Daniel; Thompson, Samantha; Triaud, Amaury H. M. J.; ... Show more Show less
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Abstract
We report on the discovery of a transiting Earth-sized (0.95R ⊕) planet around an M3.5 dwarf star at 57 pc, EPIC 249631677. The planet has a period of ~3.14 days, i.e., ~π, with an installation of 7.45 S⊕. The detection was made using publicly available data from K2's Campaign 15. We observed three additional transits with SPECULOOS Southern and Northern Observatories, and a stellar spectrum from Keck/HIRES, which allowed us to validate the planetary nature of the signal. The confirmed planet is well suited for comparative terrestrial exoplanetology. While exoplanets transiting ultracool dwarfs present the best opportunity for atmospheric studies of terrestrial exoplanets with the James Webb Space Telescope, those orbiting mid-M dwarfs within 100 pc such as EPIC 249631677b will become increasingly accessible with the next generation of observatories.
Date issued
2020-09
URI
https://hdl.handle.net/1721.1/128490
Department
Massachusetts Institute of Technology. Department of Earth, Atmospheric, and Planetary Sciences; Massachusetts Institute of Technology. Department of Physics; MIT Kavli Institute for Astrophysics and Space Research
Journal
Astronomical Journal
Publisher
American Astronomical Society
Citation
Niraula, Prajwal et al. "π Earth: A 3.14 day Earth-sized Planet from K2's Kitchen Served Warm by the SPECULOOS Team." Astronomical Journal 160, 4 (September 2020): 172 © 2020 The American Astronomical Society
Version: Final published version
ISSN
1538-3881

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