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Kepler's laws

British  

plural noun

  1. three laws of planetary motion published by Johannes Kepler between 1609 and 1619. The first states that the orbit of a planet describes an ellipse with the sun at one focus. The second states that, during one orbit, the straight line joining the sun and a planet sweeps out equal areas in equal times. The third states that the squares of the periods of any two planets are proportional to the cubes of their orbital major axes

"Collins English Dictionary — Complete & Unabridged" 2012 Digital Edition © William Collins Sons & Co. Ltd. 1979, 1986 © HarperCollins Publishers 1998, 2000, 2003, 2005, 2006, 2007, 2009, 2012

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But we can measure the distance to many other solar system objects and use Kepler’s laws to give us the distance to the Sun.

From Textbooks Oct. 13, 2016

With such a force and the laws of motion, Newton was able to show mathematically that the only orbits permitted were exactly those described by Kepler’s laws.

From Textbooks Oct. 13, 2016

We have seen that Kepler’s laws, which do not take into account the gravitational effects of the other planets on an orbit, really work quite well.

From Textbooks Oct. 13, 2016

Kepler’s laws were formulated based on observations from Brahe; however, they were not proved formally until Sir Isaac Newton was able to apply calculus.

From Textbooks Mar. 30, 2016

He also noted, though, from Kepler’s laws, that the ‘endeavours of receding from the Sun’ of the planets in their orbits were inversely proportional to the squares of their distances from the Sun.

From "The Scientists" by John Gribbin

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