PPT-Review: Newton’s 1

st amp 2 nd Laws 1 st law Galileos principle of inertia no force is needed to keep an object moving with constant velocity 2 nd law law of dynamics a n et force . 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 st. & 2. nd. Laws. 1. st. law. (. Galileo’s principle of inertia. )- no force is needed to keep an object moving with . constant velocity. 2. nd. law. (. law of dynamics. ) – a . n. et force . Laws of Motion. November 2011. Sir Isaac Newton. 1. Described 3 laws that relate forces to motion. 2. . Force. -a push or a pull, all forces have size and direction. Vocabulary. 1. . Friction. - a force that opposes motion between 2 objects that are touching. 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, . The  Newton British School  Newton British Academy   Newton International School – D - Ring Campus  Newton International School – Lagoon Campus Building . Science Champions. In thought. http://www.wimp.com/spaceshuttle/. After watching the Discovery launch, explain how Newton’s three laws are used by NASA scientist to launch a space shuttle. . st. & 2. nd. Laws. 1. st. law. (. Galileo’s principle of inertia. )- no force is needed to keep an object moving with . constant velocity. 2. nd. law. (. law of dynamics. ) – a . n. et force . The Law of Inertia. The first law says that an object at rest tends to stay at rest, and an object in motion tends to stay in motion (with the same direction and speed) unless acted upon by an unbalanced force.. Motion. Lesson 15. February 8. th. , 2011. Newton’s Second Law of Motion. If the external force on an object is not zero, the objet accelerates in the direction of the net fore. The magnitude of the acceleration is directly proportional to the net force and inversely proportional to the objects mass. . AT AGE 18 HE ENTERED TRINITY COLLEGE, CAMBRIDGE AS A SIZAR. A SIZAR WAS KIND OF A “WORK-STUDY” ASSISTANTSHIP FOR TALENTED STUDENTS FROM POOR FAMILIES. THEY PAID NO TUITION BUT HAD TO PERFORM MENIAL, SOMETIMES DEMEANING TASKS AND WERE CONSIDERED SUBORDINATE TO TUITION PAYING STUDENTS. WHILE ARISTOTILEAN PHILOSOPY WAS EMPHASIZED THERE HE PREFERRED TO STUDY DESCARTE. HE ALSO IMMERSED HIMSELF IN THE STUDY OF COPERNICUS, GALILEO AND KEPLER 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 . Whenever one object exerts a force on a second object, the second object exerts an equal and opposite force on the first.. “To every action there is an equal and opposite reaction”. F(AB) = - F(BA). Jessie Twigger. Christian Zelenka. How is this technique conducted. The Newton-Raphson formula consists geometrically of . extending the tangent line at a current point . until it crosses zero, then . nd. Laws. 1. st. law. (. Galileo’s principle of inertia. )- no force is needed to keep an object moving with . constant velocity. 2. nd. law. (. law of dynamics. ) – a . n. et force . must be applied to .