2022年2018学年高中物理人教版必修2习题:第六章万有引力与航天第3节万有引力定律2Word版含答案 .pdf

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1、名师精编优秀教案第 3 节 万有引力定律(满分 100 分,45 分钟完成)班级 _姓名 _ 第卷(选择题共 48 分)一、选择题:本大题共8 小题,每小题6 分,共 48 分。在每小题给出的四个选项中,至少有一个选项正确,选对的得6 分,对而不全得3 分。选错或不选的得0 分。1假设行星绕恒星的运动轨道是圆,则其运行周期T的平方与其运行轨道半径R的三次方之比为常数,那么该常数的大小()A只与行星有关B只与恒星有关C与行星及恒星都有关D与恒星的质量及行星的速率有关2关于地心说和日心说的下列说法中,正确的是()A地心说的参考系是地球B日心说的参考系是太阳C地心说和日心说只是参考系不同,两者具有等

2、同的价值D日心说是由开普勒提出来的3关于万有引力定律,下列说法正确的是()A天体间万有引力与它们的质量成正比,与它们之间的距离成反比B任何两个物体都是相互吸引的,引力的大小跟两个物体的质量的乘积成正比,跟它们的距离的平方成反比C万有引力与质量、距离和万有引力恒量都成正比D万有引力定律对质量大的物体适用,对质量小的物体不适用4下列说法中错误的是()A开普勒确切描述了行星的运动B牛顿发现了万有引力定律C卡文迪许测出了引力常量D阿基米德被称为称出地球质量的人5某一人造卫星绕地球做匀速圆周运动,其轨道半径为月球绕地球轨道半径的1/3,则此卫星运行的周期大约是()A14 天B48 天C816 天名师精编

3、优秀教案D16 20 天6 一个行星,其半径比地球的半径大2 倍,质量是地球的25 倍,则它表面的重力加速度是地球表面重力加速度的()A6 倍B4 倍C259倍D12 倍7设地球表面的重力加速度go,物体在距地面3R(R是地球半径)处,由于地球作用而产生的加速度为g,则ggo为()A116 B16 1 C19 D91 8月球表面重力加速度只有地球表面重力加速度的1/6,一根绳子在地球表面能拉着3kg的重物产生最大为10m/s2的竖直向上的加速度,g地 10m/s2,将重物和绳子均带到月球表面,用该绳子能使重物产生沿月球表面竖直向上的最大加速度为()A60m/s2B20m/s2C18.3m/s2

4、D10m/s2第卷(非选择题,共52 分)二、填空、实验题:本大题共5 小题,每小题5 分,共 25 分。把正确答案填写在题中横线上或按要求作答。9牛顿虽然发现了万有引力定律,却没能给出准确的引力常量。一百多年后,英国的物理学家 _巧妙地用扭秤装置,第一次在实验室里比较准确地测出了引力常量。10在太阳系中,有九大行星绕太阳运行,按照距太阳的距离排列,由近及远依次是:水星、金星、地球、火星、木星、土星、天王星、海王星、冥王星,如果把这些行星的运动近文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D

5、6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q

6、6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D

7、6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q

8、6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D

9、6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q

10、6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D

11、6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5名师精编优秀教案似为匀速圆周运动,那么它们绕太阳运行一周所用时间最长的是_,运行角速度最大的是_。11木星的公转周期为12 个地球年,设地球至太阳的距离为1 天文单位,那么木星至太阳的距离为 _天文单位。12已知月球和地球中心距离大约是地球半径的60 倍,则月球绕地球运动的向心加速度与地面上的重力加速度之比为_。13在一次测定万有引力恒量的实验里,两个小球的质量分别是0.80 kg 和 4.0 103 kg,当它们相距4.0 102 m时相互吸引的作用力是1.3 1010 N,则万有引力恒量G_Nm 2/

12、kg2。三、计算题:本大题共2 小题,计27 分。解答应写出必要的文字说明、方程式和重要演算步骤。只写出最后答案的不能得分。有数值计算的题,答案中必须明确写出数值和单位。14(12 分)如图所示,是卡文迪许扭秤实验的示意图。其中固定在T形架上的小平面镜起着非常大的作用,它利用光的反射可以把T形架的微小转动放大到能够精确测量的程度。设小平面镜到圆弧形刻度尺的距离为L,且小平面镜位于圆弧的圆心位置;T形架两端固定的两个小球中心相距为l,设放置两个大球m 后,刻度尺上的反射光点向左移动的弧长为x,那么在万有引力作用下,小球向大球移动了多少?15(15 分)月球环绕地球运动的轨道半径约为地球半径的60

13、 倍,运行周期约为27 天。应用开普勒定律计算:在赤道平面内离地面多高处,人造地球卫星随地球一起转动时,就像停留在空中不动一样(地球半径为6.4 103km)。参考答案一、选择题:文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

14、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

15、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

16、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

17、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

18、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

19、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5名师精编优秀教案1【答案】B【点拨】根据开普勒第三定律:32RkT,其中k是一个与行星无关的常数,这个常数只与中心天体有关,B正确。2【答案】AB【点拨】地心说是把地球看作静止不动

20、的,其他星体都绕地球运动,是以地球为参考系的。日心说认为太阳是静止不动的,其他行星都绕太阳匀速圆周运动,是以太阳为参考系的。两者是两种对立的观点,日心说的代表人物是哥白尼,A、B正确。3【答案】B【点拨】根据万有引力定律的内容可知,B正确。4【答案】D【点拨】根据地面上物体所受的重力等于物体与地球间的万有引力,只要测出了万有引力常量,就可求出地球质量。所以,卡文迪许被称为称出地球质量的人。D错误,本题答案为D。5【答案】B【点拨】根据开普勒第三定律可求出T5.8 天,B正确。6【答案】C【点拨】在星球表面,忽略星球的自转,认为重力等于万有引力,即2MmGmgR,得2GMgR,代入数值得0259

21、gg=,C正确。7【答案】A【点拨】物体所受的重力近似等于万有引力,2()MmGmgRh,02MmGmgR,由以上两式可得gg022()RRh116,A正确。8【答案】C【点拨】绳子能够承受的最大拉力Tmg地+ma地60N,在月球上Tmg月+ma月,有以上两式解得a月 18.3 m/s2。二、填空、实验题:文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3

22、A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:C

23、R4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3

24、A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:C

25、R4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3

26、A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:C

27、R4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5名师精编优秀教案9【答案】卡文迪许【点拨】引力常量的

28、测定是卡文迪许通过扭秤实验测出的。10【答案】冥王星;水星【点拨】根据开普勒第三定律,轨道半径越大,周期越长,角速度越小。所以,离太阳近的水星角速度大,离太阳远的冥王星周期最长。11【答案】3144【点拨】地球公转周期即一个地球年,由开普勒第三定律3322RRTT木地地木可解。12【答案】13600【点拨】在地球表面有:2MmGmgR;地球对月球的万有引力产生月球的向心加速度,有2(60)MmGm aR,两式联立得:ga 13600。13【答案】6.5 1011【点拨】由万有引力定律公式122m mFGr,通过计算可求出G值。三、计算题:14【答案】4lxL【解析】由题意知,小平面镜反射的光线

29、旋转的角度为:xL=由光的反射定律知,在入射光线方向不变的情况下,反射光线旋转的角度是平面镜旋转角度的 2 倍,故平面镜与T形架旋转的角度为:122xL=根据几何关系知,小球向大球移动的距离为:11244xxllL=。15【答案】36300km【解析】设人造地球卫星轨道半径为R1,周期为T1,卫星随着地球一起转动,若相对地面静止,则卫星的周期和地球自转的周期应相同,周期为一天。文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

30、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

31、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

32、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

33、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

34、K9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4

35、M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 Z

36、K9M7D6P3E5名师精编优秀教案设月球的轨道半径为R2,周期为T2,由开普勒定律得:33122212RRTT解得:R16.67R地卫星离地面的高度为:H R1R地 5.67 R地36300km。文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文

37、档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L

38、9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文

39、档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L

40、9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文

41、档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5文档编码:CR4T4M9Y2Q6 HY4L9B3I3A1 ZK9M7D6P3E5

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