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Archimedes' principle states that an upward buoyant force exerted on a body that is immersed partially or entirely in a fluid is equal to the weight of the fluid displaced by it. To understand how much buoyant force is needed to make an object float, let us think about what happens when a submerged object is removed from a fluid. If the object were not in the fluid, the space occupied by the object would be filled by the fluid having a weight wfl. This weight is supported by the surrounding...
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Updated: Jul 11, 2026

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1981N1:一个海王星弧?

W B Hubbard

    Science (New York, N.Y.)
    |March 14, 1986
    PubMed
    概括
    此摘要是机器生成的。

    一个1981年海王星天体,最初被认为是卫星,很可能是一个行星弧. 在亚利桑那州弗拉格斯塔夫同时进行的观测排除了卫星的存在,并限制了弧形几何.

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    科学领域:

    • 行星科学 行星科学
    • 天文学 天文学
    • 海王星系统动力学

    背景情况:

    • 1981年,在海王星附近通过恒星遮蔽探测到一个物体,最初被确定为新卫星.
    • 随后的重新解释表明,该物体可能是海王星的弧形,类似于1984年观察到的弧形.

    研究的目的:

    • 重新评估1981年海王星天体的性质.
    • 为了区分潜在的海王星卫星和行星弧.
    • 为了限制海王星弧的可能几何形状.

    主要方法:

    • 1981年同步测量恒星遮蔽的分析.
    • 来自亚利桑那州图森和亚利桑那州弗拉格斯塔夫的观测结果的比较.
    • 几何建模,以评估弧形配置的可行性.

    主要成果:

    • 1981年的物体在亚利桑那州弗拉格斯塔夫的同时观测时没有遮住这颗恒星.
    • 这一无效结果与对象作为海王星卫星的解释相矛盾.
    • 这些发现显著限制了海王星弧形的可能形状和方向.

    结论:

    • 1981年的海王星天体不太可能是卫星.
    • 这些数据支持了该物体是海王星弧的假设.
    • 这项研究为了解海王星的弧形现象提供了关键的观测约束.