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[DOCX File]Kepler's Laws lab - Mrs. Sepulveda's Classes
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Activity 2: Mercury’s Orbit (Kepler’s Second Law) In this activity, you will see if the area of a sector swept out from the Sun to Mercury remains constant between any two data points separated by EQUAL periods of time (as per Kepler’s Second Law) Choose data points 2 and 3 …
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[DOC File]Lab # 3 : Kepler's Third Law
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Kepler's three laws of planetary motion can be described as follows: Kepler’s 1st Law. The path of the planets about the sun is elliptical in shape, with the center of the Sun being located at one focus. (The Law of Ellipses) I. The orbits of the planets are ellipses, with the Sun at one focus of the ellipse.
kepler third law

[DOC File]TAP 403-2: Using Kepler's third law - Institute of Physics
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Although Kepler derived these laws for the motions of the planets around the Sun, they are found to be true for any object orbiting any other object. The fundamental nature of these rules and their wide applicability is why they are considered ``laws'' of nature. Select the image to show an animation of Kepler's 3 …
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[DOC File]Kepler’s Laws:
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Kepler’s Third Law, the “Law of Periods” relates a planet’s period of revolution (the time it takes to complete one orbit of the Sun) to its average distance from the Sun. Kepler determined the mathematical relationship between period and distance and concluded that the square of a planet’s period is proportional to the cube of its mean distance from the Sun.
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[DOC File]Kepler’s Laws
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1.) State Kepler’s 1st Law: 2.) State Kepler’s 2nd Law: 3.) State Kepler’s 3rd Law: 4.) The diagram to the right is the orbit of a comet: A) Label the two focal points. B) Label the Perihelion. C) Label the Aphelion. 5.) Mercury’s period of revolution is 88 days, or .241 years. Calculate the average distance Mercury is from the Sun. 6.
kepler's laws of planetary motion

[DOC File]Physics Unit 3 Keplers Laws
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(show sample calculations for each of the 3 columns you have to fill in) AK/NATS 1745.06 Fall 2006 . kepler. Page . Distance from the Earth's Centre (x1000km) Orbital Period (hours) Graph 1 : Kepler's Harmonic Law for Earth Satellites. 5.00 100.00 500.00 1.00 89.44 1000.00
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[DOC File]Kepler’s Three Laws of Planetary Motion - Weebly
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Kepler’s laws were formulated for elliptical orbits (of which the circular orbit is a simple special case). The ‘R’ of the third law is the semi-major axis (found as the average of the maximum and minimum distances between a satellite and the body it orbits).
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Kepler's laws of planetary motion - Wikipedia
Kepler’s laws describe common features of the motions of orbiting objects, including their elliptical paths around the sun. Orbits may change due to the gravitational effects from, or collisions with, other objects in the solar system. (HS-ESS1-4) Scale, Proportion, and Quantity .
kepler's laws derivation

[DOC File]Kepler's Laws of Planetary Motion
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Kepler’s Third Law, the “Law of Periods” relates a planet’s period of revolution (the time it takes to complete one orbit of the Sun) to its average distance from the Sun. Kepler determined the mathematical relationship between period and distance and concluded that the square of a planet’s period is proportional to the cube of its mean distance from the Sun.
kepler's laws for kids

Kepler s laws 3