PPT-Gravity and Motion: Kepler/Newton/Einstein

Astronomy Chapter 2 D Taylor 2011 2012 20132014 Gravity and Motion 2 Introduction Gravity gives the Universe its structure It is a universal force that causes all objects to pull on all other objects everywhere. Gravity Pilates Tina Gravity Danielle MIND STUDIO MONDAY TUESDAY WEDNESDAY THURSDAY FRIDAY SATURDAY SUNDAY 8:00 Spartacus Boot Camp Rick 9:30 Barre Marla/Danielle Fusion (L1-2) Naomi Hatha 1. What is Physics?. Study of the nature of the Universe. what the Universe is made of – . Matter. stars and planets and . galaxies. different forms like gases and liquids and solids. sub-atomic particles like protons and electrons. 1 = 8.85 32 = 283.22 63 = 557.60 94 = 831.97 125 = 1106.34 2 = 17.70 33 = 292.07 64 = 566.45 95 = 840.82 126 = 1115.19 3 = 26.55 34 = 300.93 65 = 575.30 96 = 849.67 127 = 1124.04 4 = 35.40 35 = 309.78 Chapter 2 Section 2 Review. A. . An object at rest remains at rest, and an object in motion remains in motion at constant speed and in a straight line unless acted on by an unbalanced force.. B. . Every action has an equal and opposite reaction. . To Cambridge University . sizar. in 1661 . Plague forced university to close – Newton goes home to . Woolsthorp. Annus. mirabilis of 1666. Calculus. Problem of the Moon. Dominated by Aristotle. Newton read Descartes, Galileo, . Steve B. . H. owell. NASA Ames Research . Center. 11-13 March 2014. Q1. -Q12 . Planet Candidates. Kepler Planet. s:. Habitable . Zone, Frequency. 3. Approximately . 50% of M dwarfs harbor a planet smaller than 1.4 R. 1571- 1630. aus Weil der Stadt. (. F. reie . R. eichsstadt). . . Amand Faessler. Kepler. Geburtshaus in. Weil der Stadt. Johannes Kepler steht in der . Reihe der größten Astronomen. Ptolemäus 150 nach Christus; . Simple version of Newton’s three laws of motion. Newton’s Laws and the Mousetrap Racecar. 3. rd. Law: “for every action there is an equal and opposite reaction”. Is more mass a good thing or a bad thing for a mousetrap racecar to go far?. fig_03_022. Nicolaus Copernicus. Copernicus’ Universe. Contrast Copernicus with the Aristotelian Cosmos. GALILEO. Galileo Galilei 1564 - 1642. Galileo's most original contributions to science were in mechanics: he helped clarify concepts of acceleration,. Housekeeping. Newton’s . First Law of . Motion. Newton’s Second Law of . Motion. Newton’s Third Law of Motion. Glossary. Inertia. is the property of objects that makes them resist changes in their motion. So, the greater the mass of an object, the more inertia it has. For example, it takes a much . starting . point. MATH. . 6630. By. . Morgan. . and . tajero. BACKGROUD. “Newton Method” is also called as Newton-Raphson Method, which been named by Isaac Newton and Joseph Raphson.. Newton Method was first published in 1685 . https://kepler.nasa.gov/images/videos/transitAnimation1.mov. KEPLER. HAS THE PRECISION TO FIND EARTHS & IT IS THE FIRST TO DISCOVER LIGHT FROM THIS PLANET. Measurement scatter is within. the line thickness.. MAHHHHZ!. © 2009. , 2010, 2011. Daryl L. Taylor, . Fizzix/. Astro. . Guy. Greenwich HS, CT . / Rowan University, NJ. DTFizzix.com. WHS. Pre-assessment :. 3. . 2. . 4. . 5. . 6. . 7. . Betty Boop . Bullwinkle J. Moose . Bormann. Honors Science - 8. Lets make some connections…. Aristotle – (384-322 BC). Nicolaus. Copernicus (1473-1543). Tycho. Brahe (1546-1601). Johannes . Kepler. (1571-1630). Galileo . Galilei.