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单词 Kepler Laws
释义

Kepler Laws

原声例句
TED-Ed(视频版)

I went to the Barnes and Noble, and I got a textbook, and from the data that was in that textbook I derived Kepler's laws.

我去了巴诺书店(译注:美国最大零售连锁书店), 拿了一本教材,根据那本书的数据, 我推导出了开普勒定理。

Crash Course 综合篇

We also talked about Kepler’s three laws, and calculated the gravitational acceleration on the surface of Mars.

我们还讲了开普勒三定律, 计算了火星表面的重力加速度。

Crash Course Physics 速成课物理

We also talked about Kepler's three laws, and calculated the gravitational acceleration on the surface of Mars.

当我们谈到开普勒三定律时, 我们计算了火星上的重力加速度。

Crash Course Physics 速成课物理

And that's what's known as Kepler's first law, and it actually applies to any elliptical

切割曲率。这被称为开普勒定律 首先,它可以应用于任何椭圆轨道。

复习

The authenticity of this story cannot be verified and in fact, it was Kepler's three laws that truly motivated the formulation of the law of universal gravitation.

这个故事的真实性无法证实,事实上,真正推动万有引力定律制定的是开普勒三定律。

英语百科

Kepler's laws of planetary motion

Figure 1: Illustration of Kepler's three laws with two planetary orbits. (1) The orbits are ellipses, with focal points ƒ1 and ƒ2 for the first planet and ƒ1 and ƒ3 for the second planet. The Sun is placed in focal point ƒ1.  (2) The two shaded sectors A1 and A2 have the same surface area and the time for planet 1 to cover segment A1 is equal to the time to cover segment A2.  (3) The total orbit times for planet 1 and planet 2 have a ratio a13/2 : a23/2.
Figure 2: Kepler's first law placing the Sun at the focus of an elliptical orbit
Figure 4: Heliocentric coordinate system (r, θ) for ellipse. Also shown are: semi-major axis a, semi-minor axis b and semi-latus rectum p; center of ellipse and its two foci marked by large dots. For θ = 0°, r = rmin and for θ = 180°, r = rmax.

In astronomy, Kepler's laws of planetary motion are three scientific laws describing the motion of planets around the Sun.

Most planetary orbits are close to being circles, and careful observation and calculation is required in order to establish that they are actually not perfectly circular ellipses. Using calculations of the orbit of Mars, whose published values are somewhat suspect, which indicated elliptical orbits, Johannes Kepler inferred that other heavenly bodies, including those farther away from the Sun, also have elliptical orbits.

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更新时间:2025/6/22 19:35:50