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[DOC File]Formula Sheet for Astronomy I - Bristol
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Law of Areas and Angular Momentum. dA/dt = rvt/2 = r2(d(/dt)/2 = H/2 = A/P = (ab/P Kepler’s 2nd law - of areas. v2 = G(m1 + m2) [2/r - 1/a] vis viva equation (velocity at any point r in orbit) vper = 2(a/P [(1+e)/(1-e)]1/2 velocity at perihelion. vaph= 2(a/P [(1+e)/(1-e)]-1/2 velocity at aphelion Newtonian Mechanics. Law of inertia
physics angular momentum equation

[DOC File]Astronomy Review Sheet - Birmingham Schools
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Pickett, M. K., Davis, G. A., & Durisen, R. H. 1993, ``The Effect of Angular Momentum Distribution and Equation of State on the Stability of Rotating Stars and Disks'', Gordon Research Conference on Origins of Solar Systems.
total angular momentum equation

[DOC File]1
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A Few Hints for 15.3.3: that first matrix element comes from adding a spin j to a spin 1, writing the usual maximum m state, applying the lowering operator to both sides to get the total angular momentum j + 1, m = j state, then finding the same m state orthogonal to that, which corresponds to total angular momentum j (instead of j + 1).
conservation of angular momentum equations

[DOC File]PHYS 228 Astronomy & Astrophysics - Widener University
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These generators are identified with energy, linear momentum, and angular momentum. That is, in any space-time model possessing space and time-translation invariance and space rotation invariance energy, linear momentum, and angular momentum must be conserved. 2. Special Relativity. The Lorentz transformation operator can be written
angular momentum and torque equation

[DOC File]D
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B. Angular Momentum or Azimuthal Quantum Number, “l” (Sublevels): Within each energy level, the electrons are located in various sublevels – there are 4 different sublevels s, p, d, and f. “l” defines the shape of the orbital (s, p, d, & f). The possible values of “l” are limited by the value for “n”.
translational angular momentum equation

Angular Momentum - Astronomy Notes
Equation of ellipse in polar co-ordinates: eccentricity: perihelion distance: Synodic period of planet, Ts, given by: Kepler’s Third Law: Angular momentum: J = Vis-viva equation: Roche limit: Hydrostatic equilibrium: Barometer equation: P = Ps exp(-mgh/kT) Thermodynamic equilibrium: T = Stars
angular momentum formula

Angular momentum equation astronomy