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Exploring Newton's Laws and Galileo's Discoveries in Motion and Gravity

Discover the predictability of the universe through Newton's laws of motion and gravity, and Galileo's groundbreaking discoveries in motion and astronomy. Learn about the scientific method, planetary movements, and the evolution of astronomical models throughout history. Explore the laws governing acceleration, velocity, and trajectories, as well as the importance of observation and measurement in scientific inquiry.

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Exploring Newton's Laws and Galileo's Discoveries in Motion and Gravity

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  1. Great Idea #2: Newton’s universal laws of motion and gravity predict the behavior of objects on Earth and in space.

  2. How Do Objects Move? Key Idea: One set of laws describes motions on Earth and in space • Universal laws of motion • The universal law of gravity Key Terms: • Force • Uniform Motion • Acceleration • Weight vs. Mass

  3. What evidence do you have that the universe is predictable?

  4. Newgrange, Ireland:5,000-year old “passage tomb”

  5. Winter Solstice

  6. Stonehenge • On the Salisbury Plain of southern England

  7. Summer Solstice

  8. What evidence do you have that the universe is predictable?“Aristotelians considered that knowledge about nature could be won by pure thought, and that experiment was, in a way, a rather trivial and pedestrian proceeding.”British Historian, Neville Andrade

  9. What evidence do you have that the universe is predictable?Oxford College—ca.1500

  10. What evidence do you have that the universe is predictable?“Galileo had thought [the discoveries of the telescope] would provide irrefutable proof to any man in good faith. … But a few months were enough to undeceive him. Certain doctors steadfastly refused to look through the telescope. … Some did look and professed to see nothing; most of them, however, said that they had never gotten around to looking through it, but that they knew already that it would show nothing of philosophical value” Historian of Science, Giorgio de Santilliana

  11. A Hierarchy of Scientific Ideas • Fact (a confirmed observation) • Hypothesis (an educated guess) • Law (a predictive mathematical description of nature) • Theory (a well established explanation of nature)

  12. The Idealized Scientific Method

  13. John Snow (1813-1858) He used the scientific method to discover that contaminated water at the Broad Street Pump was the source of a deadly cholera outbreak in London. His research saved countless thousands of lives.

  14. Measurements and Observations • How would you measure a star’s position? • Compass – direction to an object (degrees from North) • Protractor w/ straw (degrees from horizon) • Plot changes from night to night • Planets (Mars) display retrograde motion • Patterns emerge

  15. Ptolomy’s Model of the Solar System • Model of the universe with Earth at the center (13-volume Almagest) • Epicycle (wheels within wheels) • Why is it important? • Navigation • Astrology • Lasted 1500 years

  16. Dead White Males • Nicolas Copernicus (1473-1543) • Sun-centered solar system • Tycho Brahe (1546-1601) • Meticulous measurements of planet positions • Johannes Kepler (1571-1630) • Mathematical analysis of planetary orbits • Galileo Galilei (1564-1642) • Founder of experimental physics

  17. Ptolomeic vs. Copernican models • Earth- vs. Sun-centered • Perfect circles (still need epicycles) Ptolomy Copernicus

  18. Tycho Brahe (1546-1601) • Personality—Tycho’s nose • Observed a new star • Showed heavens can change over time • Designed and used new astronomical instruments • Collected data on planetary movements

  19. The Quadrant

  20. Tycho Brahe (1546-1601) • Uncertainty • before Tycho

  21. Tycho Brahe (1546-1601) • Uncertainty • before Tycho

  22. Tycho Brahe (1546-1601)

  23. Johannes Kepler (1571-1630) • Mathematician • Assistant to Tycho Brahe • Inherited his notebooks • Traditional ideas of the solar system are wrong (Kepler’s Laws)

  24. Kepler’s Laws of Planetary Motions First Law: Planets have elliptical orbits

  25. Elliptical orbits

  26. Kepler’s Laws Second Law: Orbits sweep out equal areas in equal times

  27. Kepler’s Laws Third Law: Distant orbits take longer. (Average orbital radius)3 = k (orbital period)2 R3/P2 = constant

  28. Galileo Galilei (1564-1642) • Mathematician and musician • Improved the telescope

  29. Galileo Galilei (1564-1642) • Mathematician and musician • Improved the telescope • Observational astronomy

  30. Galileo Galilei (1564-1642) • Mathematician and musician • Improved the telescope • Observational astronomy • Founder of experimental science • Arrogant and contemptuous of others • Published in Italian (vernacular) promoting Copernican view • Heretic (threatened with torture) so he recanted

  31. Galileo – The Founder ofExperimental Science Galileo studied the relationship among distance, time, velocity and acceleration He observed that objects accelerate while falling:

  32. Galileo’s Discoveries • Constant acceleration • Balls on a plane: v = at • Freefall • Constant acceleration at g • g = 9.8 m/s2 = 32 feet/s2 • Distance traveled (d) = ½at2

  33. Speed, Velocity, and Acceleration • Speed = distance traveled over time • Velocity = speed with direction • Equation for speed: • Acceleration = rate of change of velocity • Equation for velocity:

  34. Galileo’s Laws of Motion • Trajectories are parabolas • All objects fall at the same velocity • Distance of fall = k(Time)2 Remember Kepler (1571-1630) • Orbits are ellipses • Equal areas in equal times • (Radius)3 = k(Time)2 Now on to Sir Issac Newton (1642-1727)

  35. Sir Issac Newton (1642-1727) • Born prematurely • Abandoned by his mother • Forced to run family farm • Sent to Cambridge University • Made fundamental advances in several scientific fields

  36. x Cambridge

  37. Issac Newton’s – Plague Years (1665-1666) • Calculus

  38. Issac Newton’s – Plague Years (1665-1666) • Calculus 2. Laws of optics • Broke white light into colored light

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