一颗人造卫星的质量为m,离地面的高度为h,卫星做匀速圆周运动,已知地球半径为R,地球表面重力加速度为

2025-04-06 18:52:26
推荐回答(3个)
回答1:

想当年在高中最擅长物理题目了,时隔多年,依然不变,呵呵。
问题1:思路,地球对卫星的引力提供向心力,也就是引力=向心力,求出v,然后用轨道周长来计算周期(注:地球质量在高中物理是需要记忆的物理常量);22:H<3:成为近地卫星的必要速度:7.9KM/s,成为太阳卫星(行星)的速度,以及离开太阳系的最少速度这三个速度是要求会推导的(主要就是运用能量守恒的思想,推导有助于对能量定律的理解),还有就是如果速度分别介于他们之间的时候卫星的运行轨道是椭圆,这个了解就可以了,高中不要求掌握。 建议你看看高中物理竞赛,刚开始可能看不懂,但是多看,过一段时间就会豁然开朗,这对于学习高中物理相当有帮助,我当年学完高中物理竞赛后高考知识完全不用专门去复习都基本能拿满分(但是要注意不要陷入竞赛的圈子里跳不出来,因为高中物理有很多是近似求解,所以做高考物理时不要拿竞赛的审题标准去要求他)

回答2:

在地球表面:(GmM)/R^2=mg万有引力等于重力
可以用已知字母代替M(地球质量)
然后再用一次(GmM)/(R+r)^2=(r+R)4派^2/T^2 R+r是卫星做圆周运动的半径
可以求T
第2题也类似的,把H=0和=R代入r
结果应该是个范围
这种题掌握套路很简单的

回答3:

(GmM)/R^2=mg
(GmM)/(R+r)^2=(r+R)4派^2/T^2

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