摘要：Young planets offer a direct view of the formation and evolution processes that produced the diverse population of mature exoplanet systems known today. The repurposed Kepler mission K2 is providing the first sample of young transiting planets by observing populations of stars in nearby, young clusters and stellar associations. We report the detection and confirmation of two planets transiting K2-264, an M2.5 dwarf in the 650Myr old Praesepe open cluster. Using our notch-filter search method on the K2 light curve, we identify planets with periods of 5.84 and 19.66 days. This is currently the second known multi-transit system in open clusters younger than 1Gyr. The inner planet has a radius of - + 2.27 0.16 0.20 Å R and the outer planet has a radius of - + 2.77 0.18 0.20 R ⊕ . Both planets are likely mini-Neptunes. These planets are expected to produce radial velocity signals of 3.4 and 2.7m s −1 , respectively, which is smaller than the expected stellar variability in the optical (;30 m s −1 ), making mass measurements unlikely in the optical but possible with future near-infrared spectrographs. We use an injection-recovery test to place robust limits on additional planets in the system and find that planets larger than 2 R ⊕ with periods of 1–20days are unlikely.
关键词：open clusters and associations: individual;planetary systems;planets and satellites: formation;stars: low-mass
