SPHERE (87) Sylvia images
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Dynamical models of Solar System evolution have suggested that the so-called P- and D-type volatile-rich asteroids formed in the outer Solar System beyond Neptune's orbit and...
太阳系演化的动力学模型已表明,所谓的P型(P-type)与D型(D-type)富挥发性小行星形成于海王星轨道外侧的外太阳系,且……



