Science, asked by dipstaak, 10 months ago

state Kepler's all the three laws and learn them as it is​

Answers

Answered by sharmilachaudhary31
0

Answer:

In astronomy, Kepler's laws of planetary motion are three scientific laws describing the motion of planets around the Sun, published by Johannes Kepler between 1609 and 1619. The laws state that:

1) The orbit of a planet is an ellipse with the Sun at one of the two foci.

2) A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.

3) The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.

The elliptical orbits of planets were indicated by calculations of the orbit of Mars.[3] From this, Kepler inferred that other bodies in the Solar System, including those farther away from the Sun, also have elliptical orbits. The second law helps to establish that when a planet is closer to the Sun, it travels faster. The third law expresses that the farther a planet is from the Sun, the longer its orbit, and vice versa.

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Answered by AMANuchiha
2

Answer:

Hello my friend

Explanation:

Kepler devised 3 laws , they were as follows:-

1. Kepler's first law - (sometimes referred to as the law of ellipses) - explains that planets are orbiting the sun in a path described as an ellipse. ... The resulting shape will be an ellipse.

2.Kepler's Second Law, or The Law of Equal Areas in Equal Time — The line between a planet and the sun sweeps out equal areas in the plane of the planet's orbit over equal times. ... It is often called the Law of Harmony because it shows a harmonic relation between distances and periods.

3.The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit

in short

1. The orbit of a planet is an ellipse with the Sun at one of the two foci.

2. A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time.

3. The square of the orbital period of a planet is directly proportional to the cube of the semi-major axis of its orbit.

Hopefully that was helpful (。◕‿◕。)➜

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