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After Galileo

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When we Left Galileo Inquisition 1633: – “vehemently suspect of heresy” – that the Sun lies motionless at the center of the universe, that the Earth is not at its center – required to “abjure, curse and detest” – sentenced to house arrest Many scientists did not support Galileo – Difficult to see through primitive telescope – Earth obviously not moving No overwhelming evidence

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Kepler 1571-1630 Astronomer and Mathematician Assistant to Tycho Brahe Astrologer to Holy Roman Emperor Mystic – 5 Regular Solids – 5 Planets Tycho’s Data Modern Science Einstein - “God does not play dice.”

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Kepler Three Laws: The orbit of a planet is an ellipse with the Sun at one of the two foci. A line segment joining a planet and the Sun sweeps out equal areas during equal intervals of time. The square of the orbital period of a planet is proportional to the cube of the semi-major axis of its orbit. Prob Set 10C

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Newton 1642-1727 Mathematical Genius Manic-Depressive No Social Life Invented Calculus Professor at Cambridge At the Royal Society rumor of a mathematician at … “What path would a planet follow if the sun attracted it with an inverse square force?” Newton Answered: “An ellipse”

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Inverse Square Legend has it that Newton was looking at an apple a apple = 9.8 m/s 2 a moon =.0027 m/s 2 Ratio = 9.8 /.0027 ≈ 3600 Radius of earth = 6.38 * 10 6 m Radius of moon’s orbit = 3.84 *10 8 m Ratio = 3.84x10 8 / 6.38x10 6 = 60.2 60 x 60 = 3600 The moon is 60 times farther away It’s acceleration is 3600 times less

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a ~ 1 / r 2 F ~ 1 / r 2 10 times farther away, the earth’s gravity is 100 times weaker Here we are 4,000 miles from the center of the earth. If you weight 200 pounds here, 40,000 miles into space you will weigh 2 pounds a = k / r 2 a∙r 2 = k a 1 ∙ r 1 2 = a 2 ∙ r 2 2 a 1 / a 2 = r 2 2 / r 1 2 a 1 / a 2 = (r 2 /r 1 ) 2 Prob Set 15G

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In this chapter you will: Learn the nature of gravitational force. Relate Kepler’s laws of planetary motion to Newton's laws of motion. Describe.

In this chapter you will: Learn the nature of gravitational force. Relate Kepler’s laws of planetary motion to Newton's laws of motion. Describe.

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