PPT-Gravitation

Using the law of universal gravitation to gain perspective on planets moons stars and black holes What determines the force of Gravity Any two objects will exert an attractive force on one another based on the following . Chapter 5. Kinematics of Uniform Circular motion. An object that moves in a circle at constant speed, v, is said to be under uniform circular motion. . The magnitude of velocity remains constant.. The direction of velocity changes continuously.. the Gravitational Effects of Rotating Masses: The Thirring-Lense Papers 1 MASHHOON, FRIEDRICH W, HEHL, and DIETMAR S. THEISS fiir Theoretische Physik, Universitdt zu KOln, Abstract purpose of this Antoine A.J. van de Ven. Logic and Relativity Conference 2012. Space-time . vs. Space-. propertime. Space-time . vs. Space-proper. Twin-paradox visually explained. Negative Mass by symmetry . Generalized definition for Energy. thermodynamic processes, particularly, by flashes and explosions of the space matter. Ether vortexes are characterized by the power and volume, which may be of any magnitude. A funnel-shaped decrease SPH3U. Newton’s work. The acceleration of gravity must be caused by a net force, according to Newton’s 2. nd. Law.. Every particle of matter in the universe exerts an attractive force on every other particle.. avril 2012. Licence 3 - Gravitation. 1. Hervé Beust. Institut de Planétologie et d’Astrophysique . de Grenoble. avril 2012. Licence 3 - Gravitation. 2. Gravitation – Mécanique céleste. . L’interaction de gravitation. Ch 5: Thornton & Marion. Introduction. Newton, 1666. Published in Principia, 1687 (needed to develop calculus to prove his assumptions). Newton’s law of universal gravitation. Each mass particle attracts every other particle in the universe with a force that varies directly as the product of the two masses and inversely as the square of the distance between them.. General Relativity. Principle of equivalence:. There is no experiment that will discern the difference between the effect of gravity and the effect of acceleration.. Or…. Gravitational and inertial mass are equivalent.. Sections 9.1 – 9.3. Reminders. Reading quiz for Chapter 11 (Sections 1-2) due by start of class on . Tuesday.. Lab this week: Lab A7-CE – . Conservation of Energy . – due by Friday at 4 p.m.. In-class Quiz . . the. SOA City. 1. Strategies. . to. bring SOA . into. Enterprises. What. . is. SOA?. 2. Middleware . and. ESB . are. . the. . communication. . layer. They. . are. . the. . streets. . By Mr. V. Calzada & Mrs. swanson. Vocabulary. force. f. riction. m. agnetism. gravitation. Vocabulary. A . force. is any push or pull that causes an object to move, stop, or change direction. . © 2016 Pearson Education, Inc.. Goals for Chapter 6. To understand the dynamics of circular motion.. To study the unique application of circular motion as it applies to Newton. '. s law of gravitation.. © 2016 Pearson Education, Inc.. Goals for Chapter 6. To understand the dynamics of circular motion.. To study the unique application of circular motion as it applies to Newton. '. s law of gravitation.. (missions Apollo) . TERRE - LUNE . (missions Apollo). MARS. JUPITER. SATURNE. Pluton. Charon. SOLEIL. Le premier calendrier lunaire . connu. : . un os sculpté du paléolithique. . .  .                                                   .