Photometry data of (136199) Eris
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The rotational states of the members in the dwarf planet - satellite systems in the transneptunian region are determined by the formation conditions and the tidal interaction...
海王星外区域(transneptunian region)内的矮行星-卫星系统中各成员的自转状态,由其形成条件与潮汐相互作用所决定……



