General Relativity: An Introduction for Physicists · Problem 10.2

Experimental tests of general relativity — Hobson, Efstathiou & Lasenby

Physics · newtonian-orbital-solution-ellipse

Problem

Show that the equation of motion in Exercise 10.1 has the solution u=GMh2(1+ecos⁡ϕ),u = \frac{GM}{h^2}(1 + e\cos\phi), and that this describes an ellipse. Show further that a=h2GM(1−e2),a = \frac{h^2}{GM(1-e^2)}, where r1=a(1−e)r_1 = a(1-e) and r2=a(1+e)r_2 = a(1+e) are the distances of closest and furthest approach respectively.

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