TOI-1710 HARPS-N radial velocity curve
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The obliquity between a planet's orbital axis and its host star's spin axis provides crucial insights into planetary formation and migration. Planets with scaled semi-major axes...
行星轨道轴与宿主恒星自转轴之间的转轴倾角(obliquity),可为行星形成与迁移过程的研究提供关键洞察。具备尺度归一化半长轴的行星……



