14 research outputs found

    TOI-4010: A System of Three Large Short-Period Planets With a Massive Long-Period Companion

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    We report the confirmation of three exoplanets transiting TOI-4010 (TIC-352682207), a metal-rich K dwarf observed by TESS in Sectors 24, 25, 52, and 58. We confirm these planets with HARPS-N radial velocity observations and measure their masses with 8 - 12% precision. TOI-4010 b is a sub-Neptune (P=1.3P = 1.3 days, Rp=3.020.08+0.08 RR_{p} = 3.02_{-0.08}^{+0.08}~R_{\oplus}, Mp=11.001.27+1.29 MM_{p} = 11.00_{-1.27}^{+1.29}~M_{\oplus}) in the hot Neptune desert, and is one of the few such planets with known companions. Meanwhile, TOI-4010 c (P=5.4P = 5.4 days, Rp=5.930.12+0.11 RR_{p} = 5.93_{-0.12}^{+0.11}~R_{\oplus}, Mp=20.312.11+2.13 MM_{p} = 20.31_{-2.11}^{+2.13}~M_{\oplus}) and TOI-4010 d (P=14.7P = 14.7 days, Rp=6.180.14+0.15 RR_{p} = 6.18_{-0.14}^{+0.15}~R_{\oplus}, Mp=38.153.22+3.27 MM_{p} = 38.15_{-3.22}^{+3.27}~M_{\oplus}) are similarly-sized sub-Saturns on short-period orbits. Radial velocity observations also reveal a super-Jupiter-mass companion called TOI-4010 e in a long-period, eccentric orbit (P762P \sim 762 days and e0.26e \sim 0.26 based on available observations). TOI-4010 is one of the few systems with multiple short-period sub-Saturns to be discovered so far.Comment: 26 pages, 16 figures, published in A

    A Super-Earth and Sub-Neptune Transiting the Late-type M Dwarf LP 791-18

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    Planets occur 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 planets transiting the low-mass star called LP 791-18 (identified by TESS as TOI 736). This star has spectral type M6V, effective temperature 2960 K, and radius 0.17 R o, making it the third-coolest star known to host planets. The two planets straddle the radius gap seen for smaller exoplanets; they include a 1.1R ⊕ planet on a 0.95 day orbit and a 2.3R ⊕ planet on a 5 day orbit. Because the host star is small the decrease in 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

    Wolf, elk, and aspen food web relationships: Context and complexity

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