Describe briefly what the Hill radius (or distance from the secondary to the L1 equilibrium point) ells you about the extent of bound orbits about a gravitating mass.
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- Suppose an alien race on a distant planet tries to send a message to us, with a laser (light). However, we were unaware that there is a stellar-mass black hole almost directly between us and them. How would this complicate our attempts to locate their position in the Galaxy? O Gravitational lensing would make the signal appear to be coming from a different location O The information carried by the laser (light) would be altered O It would not matter The black hole absorbs all of the lightThe main mathematical tools of electromagnetism are (so far): Gauss, Stokes, Helmholtz. Write them out (in all their beauty). Don’t forget the integration boundariesGiven: ARVT and SVT are equilateral; ARVS is not equilateral. Prove: ARST is not equilateral. V R T