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星球自转角速度的上限

Upper limit of planetary rotation speed

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【作者】 于凤军汤振杰田俊龙

【Author】 YU Feng-jun;TANG Zhen-jie;TIAN Jun-long;College of Physics and Electrical Engineering, Anyang Normal University;

【机构】 安阳师范学院物理与电气工程学院

【摘要】 许多星球都有自转运动,在随星球转动的参考系中,星球的各质点受到惯性离心力的作用,使其呈现扁旋转椭球形状.转动越快,惯性离心力越大,当转速大于某临界值时星球会破裂.本文从最小势能原理出发,严格计算星球自转角速度的上限.

【Abstract】 Many planets have rotational motions. In a reference frame rotating with the planet, the mass point of the planet is subjected to an inertial centrifugal force, which makes it appear as a flat rotating ellipsoid. The faster the planet rotates, the greater the centrifugal force of inertia is. When the speed is greater than a critical value, the planet will break. Based on the principle of minimum potential energy, the upper limit of planetary rotation speed is strictly calculated.

【基金】 河南省科技攻关项目(172102210092)资助
  • 【分类号】P137;O313.3
  • 【下载频次】133
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