HARPS-N observations of K2-141 planetary system
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Ultra-short period (USP) planets are a class of low-mass planets with periods shorter than one day. Their origin is still unknown, with photo-evaporation of mini-Neptunes and in...
超短周期(Ultra-short period, USP)行星是一类公转周期短于一日的低质量行星,其起源至今尚未明确,相关研究假说包括迷你海王星(mini-Neptunes)的光致蒸发以及……



