PPT-K EPLER : the laws of planetary motion
Author : myesha-ticknor | Published Date : 2018-11-03
Physics Chapter 7Circular Motion KEPLERS FIRST LAW KEPLERS SECOND LAW KEPLERS THIRD LAW INTERESTING APPLETS Johannes Kepler Born on December 27 1571 in Germany
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K EPLER : the laws of planetary motion: Transcript
Physics Chapter 7Circular Motion KEPLERS FIRST LAW KEPLERS SECOND LAW KEPLERS THIRD LAW INTERESTING APPLETS Johannes Kepler Born on December 27 1571 in Germany Studied the planetary motion of Mars. Extra-solar planetary systems. Lecture . 16. Other theory. Tidal Hypothesis. Early attempt to explain the dichotomy of planets.. Problem?. tidal force strong enough to “draw out” a filament from stars will effectively disperse it before it could condense into planets!. Policy & REQUIREMENTS FOR . CubeSats. . Dr. Cassie Conley, James E. Johnson, . January 8, 2015. Planetary Protection Basics. Basic . w. orking. . definition - Mitigating the risks associated with microbial and organic cross-contamination,. What is a scientific theory?. . a well-supported explanation about the natural world.. . What does it really mean?. A scientific theory . EXPLAINS . WHY or HOW something happens.. Example 1:. The Big Bang Theory . Hip Special Tests Logan Dougherty. Quick Overview. Mariner 2 – First successful Venus flyby (USA). Mariner 4 – First successful Mars flyby (USA). Venera. 3 – First Venus impact. Contact lost. (USSR). Venera. 4 – Venus atmospheric probe. Background information: what students needed to know. How to calculate velocity. Newton’s 3 Laws of Motion. Kinetic and static friction. Momentum. Making sketches. EDP steps . As engineers for a toy manufacturing company, students were expected to:. 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?. Part 1. ELIZABETH MEGONIGAL. Ptolemy . (. pronouced. TAHL uh . mee. )- . 140 AD. (Greek . –. astronomer, mathematician, & geographer). He thought that . Earth was the center of the universe and the sun and the other planets revolving around Earth.. 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. Forces. We have learned that forces . either pushes or pulls.. They come in many varieties:. Gravity & Normal. Kinetic & Static Friction. Electrical & Magnetic. Air resistance. Tension. Nuclear Force. Newton’s First Law. Lesson 2. 1. . What causes an object in motion to remain in motion?. friction . inertia. gravity . velocity. 1. . What causes an object in motion to remain in motion?. Forces and Uniform Circular Motion Physics Unit 2 This Slideshow was developed to accompany the textbook OpenStax Physics Available for free at https:// openstaxcollege.org/textbooks/college-physics t. he Cosmos Mechanized. 1543. . Nicolaus Copernicus. . . - publishes heliocentric universe in De Revolutionibus Orbium Coelestium. . - implicit introduction Copernican principle: Earth/Sun is not special . Getting the Audience’s Attention. LPI Education and Public Engagement. August 22, 2018. Online Participants. Joining online? . Please share your thoughts and responses. throughout the session in the chat box..
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