kepler's law of planetary motion Synonyms
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kepler's law of planetary motion Meaning
kepler's law of planetary motion (n)
(astronomy) one of three empirical laws of planetary motion stated by Johannes Kepler
kepler's law of planetary motion Sentence Examples
- Kepler's Laws of Planetary Motion are a set of three laws that describe the motion of planets around the Sun.
- The first law states that the orbit of a planet is an ellipse, with the Sun at one focus.
- The second law states that a planet's orbital velocity varies throughout its orbit, being fastest when the planet is closest to the Sun and slowest when it is farthest from the Sun.
- The third law states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.
- Kepler's Laws of Planetary Motion were first published in 1609 by Johannes Kepler, a German astronomer and mathematician.
- Kepler's Laws were based on observations of the planets Mercury, Venus, Mars, Jupiter, and Saturn.
- Kepler's Laws were a major breakthrough in understanding the motion of planets and helped to lay the foundation for modern astronomy.
- Kepler's Laws were later used by Isaac Newton to develop his theory of universal gravitation.
- Kepler's Laws of Planetary Motion remain one of the most important and fundamental laws in astronomy.
- Kepler's Laws have been used to study the motion of planets, moons, asteroids, comets, and other objects in the Solar System.
FAQs About the word kepler's law of planetary motion
(astronomy) one of three empirical laws of planetary motion stated by Johannes Kepler
No synonyms found.
No antonyms found.
Kepler's Laws of Planetary Motion are a set of three laws that describe the motion of planets around the Sun.
The first law states that the orbit of a planet is an ellipse, with the Sun at one focus.
The second law states that a planet's orbital velocity varies throughout its orbit, being fastest when the planet is closest to the Sun and slowest when it is farthest from the Sun.
The third law states that the square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit.
