hawaiidude
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how do you calculate a planets orbit?
The discussion centers on the calculation of planetary orbits, emphasizing the use of Newtonian gravitation and the differential equation d²r/dt² = -GmMr/|r|³. Participants highlight that planetary orbits are elliptical, with the sun at one focus, and mention the significance of Kepler's laws in determining these orbits. The conversation also touches on the Lagrange points, which are relevant in three-body problems, and the leapfrog method for simulating orbits using computational techniques. Additionally, there is a request for MATLAB code to compute velocity and position vectors based on Kepler's elements.
PREREQUISITESAstronomy students, astrophysicists, and software developers interested in celestial mechanics and orbital simulations will benefit from this discussion.
Originally posted by hypnagogue
Is there any kind of physical/mechanical meaning whatsoever behind the other, non-sun focus? As far as I know there isn't, but I always wondered.
Chemicalsuperfreak wrote:Originally posted by hypnagogue
Is there any kind of physical/mechanical meaning whatsoever behind the other, non-sun focus? As far as I know there isn't, but I always wondered.
Uhh, is it one of the Lagrange points?
hypnagogue said:Is there any kind of physical/mechanical meaning whatsoever behind the other, non-sun focus? As far as I know there isn't, but I always wondered.