GCM18: The Kepler Problem

The three laws of Kepler are proved for the case of an elliptic orbit under a central force, and for the specific case of attractive gravity.

[@OzzMazz]

Very clear handwriting.

[@زينالعابدينماجدمحمد]

Excellent lecture,thank you so much sir

[@Tushar-pg2em]

Sir @1:09:18 when you write r^2, there should be eccentricity squared in RHS.
Amazing lecture by the way.. cleared all the concept of Kepler's Problem.