In this equation, "a" is equivalent to the semimajor axis of the planet's elliptical orbit (in other words the radius of its orbit, which is approximately its average distance from the Sun. Finding the "a" or radius of an object's orbit, we must assume that its orbital path is ...
Kepler's third law 英 [ˈkɛpləz θɜːd lɔː] 美 [ˈkɛplərz θɜːrd lɔː]网络 开普勒第三定律
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
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,第三速率 2.第三档,第三日 Webe...
Kepler’s Third Law is an amazing equation! It tells us that R3 T2 is the same for any planet or comet or asteroid or spacecraft that orbits the Sun. In other words, if we know a planet’s distance from the Sun, we can use Kepler’s Third Law to give us its period, or vice...
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...
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So in other words, we want to figure out T and if we have an elliptical orbit, now we're just going to use our new Kepler's Third Law equation for elliptical orbits. All right, so that's all there is to it. We're going to start out with T2=4π2a3/gm. Rememb...
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 law of planetary motion. The squares of the sidereal periods (<i>P</i>) of the planets are directly proportional to the cubes of their mean distances (<i>d</i>) from the Sun.