TOI-2000 is a metal-rich ([Fe/H] = 0.439) G-type star located about 566.2 lightyears from the solar system. The star has two hot gaseous planets, a dense mini-Neptune (b= 2.7 Re, 11 Me) and a Saturn-like planet (c= 8.14 Re, 81.7 Me). The system is optimal for the study of the formation of hot Jupiters due to the existence of the innermost planet
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