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International Solar Terrestrial Physics (ISTP) Historical Pages
If you compare the planets to the Earth (with an orbital period = 1 year and a distance = 1 A.U.), then you get a very simple relation: (a planet's sidereal period in years)2 = (semimajor axis of its orbit in A.U.)3. This is now known as Kepler's 3rd law.
kepler's laws for kids

[DOC File]Kepler's Laws of Planetary Motion
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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’s 2nd Law
third law of planetary motion

[DOC File]Kepler’s Laws:
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Answer the following questions after reviewing the “Kepler's Laws and Planetary Motion” and “Newton and Planetary Motion” background pages. Draw a line connecting each law on the left with a description of it on the right. When written as P2 = a3 Kepler's 3rd Law (with P in years and a in AU) is applicable to … any object orbiting our ...
planetary laws of motion kids

[DOC File]Jupiter and Kepler’s Laws
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Kepler’s Laws of Planetary Motion: 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 ...
kepler's laws explained

[DOCX File]Johannes Kepler: TheLaws of Planetary Motion
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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!)
kepler's 2nd law

[DOC File]PT3 Lesson Plan Rubric - ARRL - Home
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Kepler’s Third Law states that the period of a planet’s orbit squared is equal to the length of the planet’s semimajor axis cubed. For planets orbiting the Sun , where P is in years and a is in astronomical units.
johannes kepler three laws planetary motion

[DOC File]Planetary Orbit Simulator – Student Guide
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The planet will cover regions A and B is the same amount of time because of Kepler’s 2nd Law. The planet will cover region A in a faster amount of time than region B, because A has less area. The planet will take longer to move through region A because it is moving slower in region A than it is in region B. BIN 6: Meaning of Kepler’s 3rd Law
johannes kepler 3 planetary laws

[DOC File]Kepler’s Three Laws of Planetary Motion
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Kepler’s 3rd law states that the semi-major axis of a planet’s orbit (average distance to the sun in A. U.’s) is related to the planet’s orbit period (in Earth-years) by the equation: p2 = a3 Where p = orbital period in Earth years and a = distance from sun in A.U.’s.
three laws of planetary motion

[DOC File]Physics Unit 3 Keplers Laws
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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.
kepler's laws for kids

[DOC File]Lunar Events - University of Northern Iowa
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Finally they test various mathematical expressions to find a “constant” relationship between orbit period (T) and orbit radius (R) to arrive at Kepler’s 3rd Law. (All activities Kepler’s NASA) Periodic Planetary Orbits - This activity will show how to calculate the period …
third law of planetary motion

Kepler s 3rd law of planetary motion