教学讨论

星球自转角速度的上限

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  • 安阳师范学院物理与电气工程学院,河南安阳455000
于凤军( 1959—) ,男,河南安阳人,安阳师范学院物理与电气工程学院教授,主要从事理论物理、天体

收稿日期: 2018-10-02

  修回日期: 2018-12-14

  网络出版日期: 2019-07-02

基金资助

河南省科技攻关项目( 172102210092) 资助

Upper limit of planetary rotation speed

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  • College of Physics and Electrical Engineering,Anyang Normal University,Anyang Henan 455000,China

Received date: 2018-10-02

  Revised date: 2018-12-14

  Online published: 2019-07-02

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.

本文引用格式

于凤军, 汤振杰, 田俊龙 . 星球自转角速度的上限[J]. 大学物理, 2019 , 38(6) : 8 . DOI: 10.16854 /j.cnki.1000-0712.180544

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.

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