Classical Mechanics PHYS 2006 Tim Freegarde.

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Presentation transcript:

Classical Mechanics PHYS 2006 Tim Freegarde

Classical Mechanics centre of mass LINEAR MOTION OF SYSTEMS OF PARTICLES centre of mass Newton’s 2nd law for bodies (internal forces cancel) rocket motion ANGULAR MOTION rotations and infinitessimal rotations angular velocity vector, angular momentum, torque parallel and perpendicular axis theorems rigid body rotation, moment of inertia, precession GRAVITATION & KEPLER’S LAWS conservative forces, law of universal gravitation 2-body problem, reduced mass planetary orbits, Kepler’s laws energy, effective potential NON-INERTIAL REFERENCE FRAMES centrifugal and Coriolis terms Foucault’s pendulum, weather patterns NORMAL MODES coupled oscillators, normal modes boundary conditions, Eigenfrequencies

Newton’s law of Universal Gravitation Exact analogy of Coulomb electrostatic interaction gravitational force between two masses and gravitational field gravitational potential

Gravity anomaly gravity anomaly = variation from uniform solid NASA/JPL/University of Texas Center for Space Research gravity anomaly = variation from uniform solid

Gravitational attraction of a spherical shell Exact analogy of Coulomb interaction gravitational force between two masses gravitational field gravitational potential

Galilean equivalence principle gravitational field gravitational motion of mass inertial mass gravitational mass Apollo 15, David R Scott (7 August 1971) www.youtube.com/watch?v=MJyUDpm9Kvk history.nasa.gov/alsj/a15/a15.clsout3.html nssdc.gsfc.nasa.gov/planetary/lunar/apollo_15_feather_drop.html equivalence principle the trajectory of a point-like mass in a gravitational field is independent of the composition and structure of the mass inertial mass = gravitational mass

Newton’s law of Universal Gravitation Exact analogy of Coulomb electrostatic interaction gravitational force between two masses and gravitational field gravitational potential

Elliptical orbit eccentricity constant semi latus rectum polar equation Cartesian equation semimajor axis semiminor axis total energy

Conic section orbits eccentricity constant semi latus rectum polar equation Cartesian equation semimajor axis semiminor axis total energy

Conic section orbits http://www.personal.psu.edu/smh408/

Conic section orbits Alastair Rae

Conic section orbits Magnus Manske

Kepler’s laws Planetary orbits are ellipses with the Sun at one focus The radius vector from Sun to planet sweeps out equal areas in equal times The square of the orbital period is proportional to the cube of the semimajor axis