iclicker Astronomy 122 Outline

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Astronomy 1 This Class (Lecture 8): How to make a jump shot? Next Class: What is a star? iclicker There are about 5 people without iclicker registration. Register now! After Friday, only registered grades will count. If you see zeros for lecture participation (e.g. 4-Jan), see me or email me ASAP. Homework #3 due Sun at 11:59pm! Music: Earthbound Darrin Drda HW Outline As I can tell when you look at the HW, I have noticed that on Wednesday, the discussion section day, less than 5% of you have even looked at the HW-short. This makes me sad! So, I will check this again next week, if it is the same percentage, I will move the HW due to Friday evening. If it still does not improve, I will move it to Thursday morning. Don t make me sad. Before we start stars, let s talk about gravity it not just a good idea, it s the law

The Laws of Motion Until the mid-17 th century, scientists worked empirically Building a mathematical formula that fit the data No reason why the Universe worked Isaac Newton (164-177) Developed fundamental laws of nature Gave us a reason why the Sun-centered system works GRAVITY Designed the reflecting telescope Discovered that white light is a mix of all colors Also invented calculus Newton's 1 st Law of Motion Law of Inertia An object at rest will remain at rest and an object in motion will remain in motion in a straight line at constant speed, unless acted upon by an unbalanced force. What is a Force? No, not THE Force Force in the simplest sense is a push or pull. It may be from gravity, electrical, magnetic, or muscle efforts Measured in Newtons You must learn the ways of the force.

Why was it so hard to see this? A Feather and a Hammer Usually we have Friction! Friction is a possible net outside force that Newton was talking about! Remember the feather/hammer experiment? http://www.hq.nasa.gov/office/pao/history/alsj/a15/a15v_16706.mpg Newton's nd Law of Motion Law of Acceleration The net force acting on an object is proportional to the object s mass and its resulting acceleration. F = m a Acceleration is a change in velocity (in speed and/or direction, think of the 1st law) Measured in meters per second per second To accelerate something you have to apply a force Mass is amount of matter in an object Measured in grams or kilograms, not pounds! Elephant at rest stays at rest Takes a big force, or the Elephant stays at rest. Or an anvil in space even if it is weightless. http://sol.sci.uop.edu/~jfalward/physics17/chapter/chapter.html

Newton's 3 rd Law of Motion Law of Action- Reaction Every action has an equal and opposite reaction Action: Guy jumps forward out of the boat Reaction: Boat moves away from the pier Newton's 3 rd Law of Motion Law of Action- Reaction Every action has an equal and opposite reaction Action: Player makes a shot. Reaction: He moves backwards slightly. Question You are an astronaut taking a space walk to fix your spacecraft with a hammer. Your lifeline breaks and you are left floating in space. To return safely to your spacecraft, you should a) Throw the hammer at the spacecraft to get someone s attention. b) Throw the hammer away from the spacecraft. c) Use a swimming motion with your arms & legs. d) Reach down and kiss your ship goodbye. e) Cry, because you should have brought a radio with you. Newton Principia is one of great science works. By demonstrating that the motion of all bodies was controlled by the same universal laws, Isaac Newton brought to the scientific community a vision of an orderly, harmonious universe. http://www.lib.udel.edu/ud/spec/exhibits/treasures/science/newton.html

Going in a Circle Circle (or orbit) not equal to a straight line. The object is constantly changing direction. Newton and the Planets Newton s ideas can/should be applied to the heavens as well as the Earth. Right? Planetary Motion By Newton A planet going around the Sun (or a moon going around a planet) is always accelerating The direction of motion is changing There must be a force acting on the planet! (F = ma) Imagine it as a string If we cut the string, what happens? According to Newton s 1 st Law, the ball moves in a straight line Nature of Gravity Newton's Law of Acceleration then tells us that the Sun MUST be applying a force Ah GRAVITY!

Newton's Law of Gravity Any two masses have a gravitational force between them: m1m F = G r m 1 and m are the masses r is the distance between the two masses G is the gravitational constant (G = 6.67 x 10-11 when kg and meters are used) Inverse Square Law Strong function of separating distance! Half the distance makes four times the force! Newton's Law of Gravity Two bodies attract each other with a force that is directly proportional to the product of the their masses and inversely proportional to the square of the distance between them. Newton s Universal Law of Gravity The Earth pulls you and you pull it. But the Earth wins, inertial-wise. F 1 = m 1a 1 F 1 = F F = m a

What is Weight? What we feel as weight is actually the force we feel from Newton s Law of Gravity. Weight = GM R Earth M Earth you F = m a F = m a It is confusing since social convention has made weight and mass the same at the earth s surface, but what happens to your weight elsewhere? Question When you fly in an airplane, does your weight Question When you fly in an airplane, does your mass a) Increase. b) Decrease. c) Stay the same. a) Increase. b) Decrease. c) Stay the same.

Weight in an Airplane? When you fly in an airplane, you increase your distance from the center of the Earth. If the distance increases, your weight is reduced. Weight ( R 1 Earth + d) Gravity on the Moon Is there gravity on the moon? Yes! But your weight is 1/6 th of your Earth weight See you next fall.. Moon Gravity Moon weight The Moon is around 3.7 times smaller and 81 times lighter than the Earth GM Weight = R M Moon Moon you Your mass would be exactly the same, but your weight would be around 1/6 th of your weight on Earth. http://btc.montana.edu/ceres/html/weight/weightstudentactivity.htm

Moon weight Moon weight Weight = GM Moon Moon R M you = M Earth G M 81 REarth 3.7 you Weight = GM Moon Moon R M you = M Earth G M 81 REarth 3.7 you or = 1 81 GM Earth you ( 3.7) WeightEarth R M Earth 1 6 Moon Olympics? Newton's Great Insight The same force makes things fall down on Earth and keeps the planets in their orbits Orbiting bodies are falling bodies! http://www.astronomy.org/programs/moon/moon.html Or http://spaceplace.jpl.nasa.gov/orbits1.htm

Why was this important? Remember, the ancients believed that there were two sets of rules One for Earth One for the Heavens Newton showed that the same laws of nature applied everywhere! Earth is not a special place We are a part of the Universe Zero-G Why are astronauts weightless when in orbit? Are they out of the Earth's gravity? No! Gravity is what keeps them in orbit Astronauts feel weightless because they are falling at the same speed as the spacecraft There is no force pressing them against the floor Free Falling Objects Testing: Halley s Comet Halley s Comet was known to often reappear. Edmund Halley used Newton s formulism to find next arrival. Bayeux Tapestry weightless : not beyond influence of gravity Astronaut is just another orbiting body Earth s pull is what keeps astronaut in orbit Astronaut feels weightless because she and spacecraft are experiencing gravity together http://seds.lpl.arizona.edu/nineplanets/nine planets/halley.html http://www.getty.edu/artsednet/resources/space/stories/h alleys.html

Problem with Gravity? Problem with Gravity? 1830's: Uranus observed orbit did not follow predictions of Newtonian solar system model. Was this the death of Newton's gravity? Not good. Theory has to agree with all data, not just some. So despite great job with planets, moons, other stars, even one clear failure is enough. What s going on? What do you think? Throw out Newton? Unknown mass, right at predicted location in 1846. Victory snatched from jaws of defeat!!!! http://lyra.colorado.edu/sbo/hubble/ss/ss.html http://lyra.colorado.edu/sbo/hubble/ss/ss.html Escape Velocity We talked about the horizontally aimed cannon, but if we fired it vertically, what velocity do we have to fire it so that it doesn t fall back down? At some velocity the cannonball outruns gravity s pull. That number is 11. km/s or 5,000 m/hr. Astronomy: The Big Picture Seeing how all these pieces fit together into a coherent picture of our Universe! Jules Verne: Moon Ship http://vesuvius.jsc.nasa.gov/er/seh/earlysf.html

The Big Picture Star s Physical Today, we can observe in almost every part of the electromagnetic spectrum Only 100 years ago, we were blind to the big picture of the Universe As we begin to piece together the big picture, our understanding of the cosmos grows Please step on scale. Turn head. Cough. No, really. How to measure the properties of objects that are very, very far away? What properties would we like to know about the stars. http://www.pemed.com/physof/scale.jpg Star s Physical Distance Are all stars the same? Are they all just like our Sun? Do they have different brightnesses? Do they have different temperatures? Colors? Do they have different masses? Do they have different sizes? What happens to them? Just grow old and get retirement? We know that the stars must be very far away. They don t move much. Measuring the distance is a hard problem. We ve only had the technology to do it for the last 00 yrs or so.

Leaving Home Nearest star is 4 x 10 13 km away Called Proxima Centauri Around 4 light years More than 5000 times the distance to Pluto Walking time: 1 billion years Fastest space probes: Voyagers 1 &, Pioneers 10 & 11) 60,000 years at about 3.6 AU/year (38000 mi/hr) Our Nearest Neighbors http://www.anzwers.org http://antwrp.gsfc.nasa.gov/apod/ap010318.html Parallax How do astronomers measures distances to nearby stars? 1. Close one eye Stupid Demo #?. Hold out arm at full length 3. Place my face under your thumb 4. Now, switch eyes. Blink back and forth a few times. 5. Hold out arm at half-length 6. Repeat http://www.ibiblio.org/john/photos/thumb.jpg

Parallax Is Triangulation If one loses the use of an eye, then it becomes very difficult to judge distances. Usually, each of your eyes observe objects with slight shifts in position. When objects are closer, the effect is larger. Stereo-vision! http://www.kidsdomain.com/holiday/halloween/clipart/eyes.jpg