Johannes kepler s 3rd law of planetary motion

• [DOCX File]Florida State University School

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  Kepler’s 3rd Law of Planetary Motion The a planet is to the sun, the is. An orbital period is the time it takes for a planet to complete one orbit around the sun in Earth years.

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• [DOC File]Jupiter and Kepler’s Laws

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  Observe the motion of Jupiter’s moons over several days (movie) Estimate the orbiting period (T) of Moon I or II . T = Estimate the mean radius (r) of the moon’s orbit by comparing it to the diameter of Jupiter (142984 km) r = Solve for the mass of Jupiter using Kepler’s 3rd law (use consistent units!)

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• [DOC File]Lab # 3 : Kepler's Third Law

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  Johannes Kepler derived, early in the 17th century, the geometry of the planetary orbits. Of particular interest here is the Harmonic Law, which may be written in algebraic form as : where is the period of revolution of the planet, a is the . semi--major axis of the planet's orbit

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• [DOCX File]Johannes Kepler: TheLaws of Planetary Motion

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  Kepler's Third Law implies that the period for a planet to orbit the Sun increases rapidly with the radius of its orbit. Thus, we find that Mercury, the innermost planet, takes only 88 days to orbit the Sun but the outermost planet (Pluto) requires 248 years to do the same.

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• [DOCX File]Name:

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  Name: Date: Period: Kepler's Laws of Planetary Motion Introduction. Johannes Kepler published three laws of planetary motion, the first two in 1609 and the third in 1619. The laws were made possible by planetary data of unprecedented accuracy collected by Tycho Brahe.

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• [DOCX File]Unit B - DYNAMICS

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  Kepler's 3rd Law, which states the mathematical relationship between the periods of orbit, T, and the radius of orbit, R, is given by: Kepler's Constant, K, holds for all planetary bodies orbiting around the same central body or mass, so if you work out K for one planet in the solar system, you can apply this K to all other planets in the solar system to derive their periods of orbit or radius.

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• [DOC File]Chapter 2: The Science of Life in the Universe

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  Kepler's 3rd Law of planetary motion states that A) the orbits of planets are ellipses with the Sun at one focus B) an imaginary line joining the Sun and planet sweeps out equal areas in equal times C) the further a planet is from the Sun, the slower it moves in its orbit D) the further a planet is from the Sun, the faster it moves in its orbit

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