Kepler s 3rd law explained
[DOC File]Introduction to Circular Motion
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Kepler’s Three Laws. Who proposed the three laws of planetary motion? What is Kepler’s 1st law of planetary motion? What is Kepler’s 2nd law of planetary motion? Draw a picture to show how any planet sweeps out equal areas in equal amounts of time. What is Kepler’s 3rd law of planetary motion? Centripetal Force (Fc) What is centripetal ...
[DOC File]Chapter 29 Our Solar System-Planet Overview
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Explain Kepler’s 1st Lae and its relationship to the following terms . astronomical unit, perihelion, aphelion, focus, major axis, semi-major axis, the Sun, and . eccentricity. Determine the relative shape (elongated oval, oval, circle) of an orbit when given its eccentricity value. Explain Kepler’s 2nd and 3rd …
[DOC File]VPython Modeling
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Recalculate the required delta v and angles to make the Apollo spacecraft undergo a transfer orbit to the moon while the moon is moving. (Give a detailed derivation of how you obtained the launch angle. Hint since the speed of the moon is (γ/B)1/2 and the travel time can be found from Kepler’s 3rd law…
[DOC File]What Did We Used to Think About the Solar System
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Kepler (Tycho’s assistant) explained the unexpected occurrences by suggesting that the planets’ orbits were elliptical. Kepler’s . 1st law of planetary motion → _____ _____ Kepler’s . 2nd law …
[DOC File]Haverford College Fall 1993
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This law states that the period of a planet’s orbit is related to the average distance of that planet from the Sun by: P2 = a3, where P is the period of the planet’s orbit in Earth years and a is the distance from the Sun in Astronomical Units (which is the distance of the Earth from the Sun).
[DOC File]Physics Unit 3 Keplers Laws
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Forces at a distance are explained by fields (gravitational, electric, and magnetic) permeating space that can transfer energy through space. ... to arrive at Kepler’s 3rd Law. (All activities Kepler’s NASA) Periodic Planetary Orbits - This activity will show how to calculate the period of the orbit (length of the year) for planets in the ...
[DOCX File]Florida State University School
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Ptolemy explained retrograde motion by saying the planets moved along smaller circles, which in turn moved along orbits around the Earth. ... Kepler’s 2nd Law of Planetary Motion. ... Kepler’s 3rd Law of Planetary Motion. The a planet is to the sun, the is.
[DOC File]CHAPTER TWO - Physics & Astronomy
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It is only from the study of binary star orbits that the masses of stars can be calculated using Sir Isaac Newton’s (1687/1995) variation of Johannes Kepler’s (1619/1995) 3rd Law of Planetary Motion, M1 + M2 = a3/P2, where M1 & M2 are the masses of the two stars in terms of the Sun’s mass, a is the semi-major axis of the relative orbit in astronomical units (mean distance between the Earth and Sun), and …
[DOC File]Science RWLO Template Title Placeholder
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Introduce Kepler’s 3rd law: the square of the orbital period of a planet is directly proportional to the cube of the average distance of the planet from the Sun; that is,. To simplify the derivation, we will use circular orbit for the planets. The centripetal force Fc necessary …
[DOC File]Kepler's Laws of Planetary Motion
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This is now known as Kepler's 3rd law. For example, Mars' orbit has a semi-major axis of 1.52 A.U., so 1.523 = 3.51 and this equals 1.872. The number 1.87 is the number of years it …
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