Classical and celestial mechanics 0800-PA-CELMECH

(po angielsku) Contact hours with teacher: • participation in lectures - 30 hrs • participation in exercises - 30 hts Self-study hours: • preparation for lectures - 15 hrs • preparation to exercises – 30 hrs • preparation to midterm exams - 30 hrs • preparation to the final exam - 15 hrs Altogether: 150 hrs (5 ECTS)

(po angielsku) W1: the basic Newtonian classical mechanics with the focus at the N-body problem and its variants (the planetary problem) W2: the kinematics and dynamics with application of the two-body problem in astrophysics (star-planet, binary stars, planet-moon configurations) W3: the basic theory of the restricted three body problem and its selected application in astrodynamics, galactic dynamics and planetary systems W4: elements of the dynamical systems theory (K_W01, K_W03)

(po angielsku) U1: use of parametrisation of the Keplerian orbits, various types of orbital elements, propagation of the initial condition U2: construction of the kinematic merit function for astrophysical observations of binary systems (radial velocities, astrometry, eclipse timing) U3: numerical integration of the equations of motion (K_U01, K_U02, K_U04)

(po angielsku) K1: understanding the fundamental links between the mathematical theory and observations K2: understanding the significance of the Copernicus revolution K3: preparation to studying specialized subjects of astronomy (K_K02)

(po angielsku) Expository teaching methods: • informative (conventional) lecture • classic problem • exercise method

przedmiot obligatoryjny

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