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Kepler's third law 英 [ˈkɛpləz θɜːd lɔː] 美 [ˈkɛplərz θɜːrd lɔː]网络 开普勒第三定律
英英释义 a law stating that the ratio of the square of the revolutionary period (in years) to the cube of the orbital axis (in astronomical units) is the same for all planets 访问沪江小D查看kepler's third law的更多详细解释>相关短语 law of Guldberg and waage (质量作用定律) 古德柏和瓦治...
网络开普勒第三定律 网络释义 1. 开普勒第三定律 王辉:雅思阅读背景文章‘金星... ... synodic periods [天]会合周期Kepler's third law开普勒第三定律the solar system 太阳系 ... train.eic.org.cn|基于26个网页
Newton's third law 牛顿第三定律 Kepler law 【化】 开普勒定律 newton's third law of motion phr. 牛顿第三运动定律 相似单词 Kepler n. (在月球东北象限的)开普勒环形山(直径为35公里) kepler n.(在月球东北象限的)开普勒环形山(直径为35公里) third num. 第三,三分之一 n. 1.六十分之一秒...
Kepler's third law of planetary motion. The squares of the sidereal periods (P) of the planets are directly proportional to the cubes of their mean distances (d) from the Sun. © Encyclopædia Britannica, Inc./Patrick O'Neill Riley...
In the previous reading selection from Part I of Book IV of the Epitome of Copernican Astronomy, Kepler argued that it would be most fitting for the sun to be located at the center of the World, fromdoi:10.1007/978-1-4939-1360-2_16Kerry Kuehn...
Kepler’s laws apply not just to objects circling the Sun, of course, but to any object orbiting any other object due to the force of gravity. The constant C may change for different orbital systems, but Kepler’s laws are true anywhere! Kepler’s Third Law is used over and over...
According to Kepler's third law,the orbital period T of a planet is related to the radius R of its 相关知识点: 试题来源: 解析 即T ^ 2=t ^ 2 * R ^ 3 / r ^ 3 (R / r=4.97,故R ^ 3 / r ^ 3 =122.763473) 两边开方:T=t * (R ^ 3 / r ^ 3) ^ 0.5=11.07986791 (years...
Kepler's third lawKepler's third law of planetary motion. The squares of the sidereal periods (P) of the planets are directly proportional to the cubes of their mean distances (d) from the Sun. The Linz authorities had anticipated that Kepler would use most of his time to work on and ...