'Central force field' presentation slideshows

Lec 4, Friday 17 Feb

Lec 4, Friday 17 Feb. potential and eqs. of motion in general geometry Axisymmetric spherical . Laplacian in various coordinates. Example: Energy is conserved in STATIC potential. The orbital energy of a star is given by:. 0 since and. 0 for static potential.

744 views • 49 slides

509 views • 38 slides

Satellite observation systems and reference systems (ae4-e01)

Satellite observation systems and reference systems (ae4-e01). Orbit Mechanics 2 E. Schrama. Contents. Perturbed Kepler orbits Linear C20 perturbations and classification of orbits Orbit determination, solve the equation of motions Effects of other acceleration models

485 views • 33 slides

Apsidal Angles & Precession

Apsidal Angles & Precession. Brief Discussion! Particle undergoing bounded, non-circular motion in a central force field ? Always have r 1 < r < r 2 V(r) vs r curve ? Only 2 apsidal distances exist for bounded, noncircular motion. . ? - ? ?.

456 views • 10 slides