Lagrangian Point
Geostationary orbit, Centripetal force, Center of mass, Rotating reference frame
978-613-7-25612-1
613725612X
84
2011-10-03
34.00 €
eng
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Please note that the content of this book primarily consists of articles available from Wikipedia or other free sources online. The Lagrangian points (also Lagrange points, L-points, or libration points) are the five positions in an orbital configuration where a small object affected only by gravity can theoretically be stationary relative to two larger objects (such as a satellite with respect to the Earth and Moon). The Lagrange points mark positions where the combined gravitational pull of the two large masses provides precisely the centripetal force required to rotate with them. They are analogous to geostationary orbits in that they allow a relatively small object to be in a fixed position relative to one or two more massive bodies.
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