Kepler s laws 2

    • Kepler's Laws

      Unit 2 Kepler’s Laws of Orbits Name _____ Period_____ Kepler’s 2nd Law of Planetary Motion: Law of Area. 6. Observe the following diagram. This shows an elliptical orbit of a planet around the sun. Determine the AREA of the two shaded areas by counting the number of shaded squares.

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    • [DOC File]Kepler’s Laws:

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      After completing these three activities, you will better understand Kepler’s Laws and the impacts they have on planetary motion. Activity 1: Mercury’s Orbit (Kepler’s First Law) In this activity, you will be plotting the orbit of Mercury around the sun using data taken …

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    • [DOC File]BACKGROUND INFORMATION

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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.

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    • [DOCX File]GOD & MATH: Thinking Christianly About Math Education

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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 …

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    • [DOC File]Kepler’s Laws

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      Kepler’s Laws of Planetary Motion. Johannes Kepler (1571 – 1630)Born in Weil der Stadt, Württemberg, Holy Roman Empire (now Germany)Johannes Kepler was a German mathematician and astronomer who discovered that the Earth and planets travel about the sun in elliptical orbits. He gave three fundamental laws of planetary motion.

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    • [DOC File]Kepler's Laws of Planetary Motion

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      Kepler’s Second Law, the “Law of Equal Areas” states that a line drawn from the Sun to a planet sweeps equal areas in equal time, as illustrated on the diagram below. A planet’s orbital velocity (the speed at which it travels around the Sun) changes as its position in its orbit changes.

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