A super-Earth and sub-Neptune transiting the late-type M dwarf LP 791-18.
2019
Planetsoccur most frequently around cool dwarfs, but only a handful of specific examples are known to orbit the latest-type M stars. Using TESS photometry, we report the discovery of two
planetstransiting the low-mass star called LP 791-18 (identified by TESS as TOI 736). This star has spectral type M6V,
effective temperature2960 K, and radius 0.17 R_Sun, making it the third-coolest star known to host
planets. The two
planets
straddlethe radius gap seen for smaller
exoplanets; they include a 1.1 R_Earth
planeton a 0.95 day orbit and a 2.3 R_Earth
planeton a 5 day orbit. Because the host star is small the loss of light during these
planets' transits is fairly large (0.4% and 1.7%). This has allowed us to detect both
planets' transits from ground-based photometry, refining their radii and orbital ephemerides. In the future, radial velocity observations and transmission spectroscopy can both probe these
planets' bulk interior and atmospheric compositions, and additional photometric monitoring would be sensitive to even smaller transiting
planets.
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