The young HD 73583 (TOI-560) planetary system: Two 10-M mini-Neptunes transiting a 500-Myr-old, bright, and active K dwarf
arXiv:2110.13069 · doi:10.1093/mnras/stac638
Abstract
We present the discovery and characterisation of two transiting planets observed by \textit{TESS} in the light curves of the young and bright (V=9.67) star HD73583 (TOI-560). We perform an intensive spectroscopic and photometric space- and ground-based follow-up in order to confirm and characterise the system. We found that HD73583 is a young (~Myr) active star with a rotational period of \,d, and a mass and radius of and , respectively. HD73583 b ( d) has a mass and radius of and, respectively, that gives a density of . HD73583 c () has a mass and radius of and , respectively, this translates to a density of . Both planets are consistent with worlds made of a solid core surrounded by a volatile envelope. Because of their youth and host star brightness, they both are excellent candidates to perform transmission spectroscopy studies. We expect ongoing atmospheric mass-loss for both planets caused by stellar irradiation. We estimate that the detection of evaporating signatures on H and He would be challenging, but doable with present and future instruments.
Accepted for publication in MNRAS
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