Goal: To understand how Galileo and Newton used experimentation and theory to further the fields of physics and astronomy. Objectives: 1) To learn about the discoveries of Galileo. 2) To understand what made Galileo great. 3) To understand how Galileo’s findings led to the acceptance of Kepler’s Laws 4) To learn about the accomplishments of Newton. Galileo Intro (1564-1642) • Kepler’s sun centered universe was still not universally accepted. • It was still untested after all. • There were 3 main arguments against Kepler’s model: 1) Aristotle held that if the earth DID move, that birds, clouds, ect. would be left behind. 2) This contradicted Aristotle’s claim that the heavens must be perfect and unchanging. 3) If the earth really did orbit the sun, then you would be able to see stars move back and forth over the course of the year due to stellar parallax, which NOBODY had observed! Which of the following does Galileo get “credited” for? For each a = yes, b = no • • • • • • • • • 1) Mountains on the Moon. 2) Sunspots 3) rotation of the sun 4) the phases of Venus 5) 4 moons of Jupiter 6) The Milky Way was in fact a collection of stars. 7) Invention of the telescope 8) First to see Neptune 9) Discovered that gravity accelerates all objects at the same rate, regardless of mass. 1) Mountains (and craters) on the Moon. • Galileo was the first to document the mountains and craters on the moon (although someone found them just earlier, but was unable to document them). • Galileo was able to spot the shadows the mountains caused allowing him to know what they were. • Galileo’s ability to draw clearly and artistically allowed everyone to see what he could see in his telescope. • Mountains and craters were seen as imperfections. Sunspots • While the ancient Chinese reported spotting Sunspots long ago, it was neither documented nor known to Europe. • Galileo was the first to document the sunspots (by doing something you should never ever do, look at the sun through an unfiltered telescope). • The cause was unknown, but the sunspots were seen as blemishes on the sun. Rotation of the sun • By watching the sunspots, he would notice them move around the sun in about a 26 day period. • This was the rotation of the sun and 26 days is the rotational period! Phases of Venus • Venus was known to stay within about 40 degrees of the sun (and Mercury even closer). • By this time, the phases of the moon were understood to be caused by the sun’s orientation to the moon in the sky. • If Venus orbited the earth, you would only expect crescent phases of Venus. • Galileo discovered Venus went through ALL the phases! • This meant that Venus MUST be orbiting the sun. Galilean moons of Jupiter • • • • Discovered the 4 largest moons of Jupiter. Observed that they orbit around Jupiter! Jupiter was its own mini solar system! Not everything orbits the earth! The Milky Way • Galileo turned his telescope towards the cloudy patch known as the Milky Way. • What he saw was a field of lots and lots of tiny stars. • He concluded that these stars had to be more distant that the stars you can see with your naked eye. • Also, this could mean that the distance to the known stars is probably much higher than expected, and therefore too large to be measurable with stellar parallax. Invention of the telescope. • Galileo was certainly the first to use the telescope for astronomical purposes. • Galileo in fact had a better model of telescope than had been around. • However, the telescope itself was invented much earlier to use as a spyglass. • Galileo did not invent the telescope, and does not get credit for it although it is a common misbelief that he does. First to actually view Neptune. • Neptune was discovered much later. • However, one night Galileo was observing Jupiter at a time when Neptune was very close to it. • Galileo reported a weird blue star that appeared to move a little. • However Galileo was more preoccupied with Jupiter so did not go back to further inspect this funny blue “star”. • Therefore, Galileo made the first known observation of Neptune. Discovered that gravity accelerates all objects at the same rate, regardless of mass • True! • As long as you can remove wind resistance… • He tested this by dropping things from the top of the Leaning Tower of Pisa. • He found that everything hit the ground at the same time. • He dropped from differing heights, and measure the time it took to hit the ground in order to calculate the acceleration. • Acceleration was constant! • This made him the father of experimental physics! • Other experiments showed that things also remained in motion UNLESS some force slowed them – so birds could remain with the earth. Galileo’s reward: • Catholic church shunned him. • His book was banned. • 6/22/1633 brought before an inquisition where Galileo was forced, under penalty of death if he did not, to recant his findings. • Galileo’s Book was unbanned in 1824. • Galileo vindicated in 1992. Isaac Newton (1642-1727) • Newton was the father of theoretical physics! • Had some mathematical discoveries such as calculus. • Created “classical mechanics” – branch of physics. • Used a prism to prove that white light was actually a combination of many colors of light – lead to his book on optics. • Came up with his 3 laws of motion. Newton’s Laws: • Law 1: Law of Inertia A body in rest stays at rest until acted upon by an outside force, and a body in motion remains in motion until acted upon by an outside force. • Law 2: Force Law Force = mass * acceleration • Law 3: the Law of Action and Reaction Whenever one body exerts a force on a 2nd body, the 2nd body exerts an equal and opposite force on the first body. Universal law of gravity • • • • Realized that gravity was universal! F = G m M / r2 G is the gravitational constant. This displaced the long standing believe that physical laws on Earth and in the heavens were different somehow. • It explained the reason for the motions of the planets around the sun. • Was able to derive Kepler’s Laws, and in doing so validating and verifying BOTH theories. Universal law of gravity - questions • F = G m M / r2 • How does the magnitude of the force of gravity on me by the earth compare to the force I exert on it? • A) Same • B) Earth does far more • C) I do far more Universal law of gravity - questions • F = G m M / r2 • What is the gravitational acceleration on an astronaut at low earth orbit (~200 km above the surface or 6600 km above the center of the earth) if the acceleration of the surface of the earth is 9.8 m/s2? • A) 0 m/s2 • B) 9.2 m/s2 • C) 10.4 m/s2 • D) None of the above (i.e. very tiny or really big) Universal law of gravity - questions • F = G m M / r2 • If you double your distance from an object how does the force change? • A) Doubled • B) Halved • C) Stays the same • D) Quartered • E) gets 4 times larger Which of the following is true: A) Apples fall faster than pears. B) Gravity only exists on the surface of an object. C) Gravity extends outward far beyond the earth. D) Gravity at large distances creates a repulsive force which keeps everything from crashing into the sun. Newtonian Telescope! • Created a far superior version of the telescope (so superior it is the most widely used by professionals 300 years later). • This is a reflecting telescope. • Previous telescopes were refracting (refract light through a lens). This creates “chromatic abrasion”. Conclusion • Where Kepler left off on his observational astronomy Galileo picked up with his experimental astronomy, and Newton finished with his theoretical astrophysics. • It took all 3 to put the notion of a Earth centered system to rest at long last.