Adapted From Fundamentals of Astrodynamics and Applications, Second Edition by David A. Vallado (Vallado Orange Book)
Note! This is not an exact copy of the front cover. I have made changes to symbols where appropriate for legibility and such. For instance, I use θ {\displaystyle \theta } (theta) instead of ν {\displaystyle \nu } (nu) for true anomaly, as it looks too much like v {\displaystyle v} velocity. Go ahead and try it out! ν v v ν v ν ν v {\displaystyle \nu vv\nu v\nu \nu v} . Also, I use the same symbol E {\displaystyle E} for elliptic, parabolic, and hyperbolic eccentric anomaly. They are all used the same way, and it is always clear from context which is which.
I also group things differently, and I add in a couple of equations which are in pencil in my book.
These are provided pretty much without comment, as a reference for someone who knows what to do with the equation, but just needs to see it written out.
sin E = s i n θ 1 − e 2 1 + e cos θ {\displaystyle \sin {E}={\frac {sin{\theta }{\sqrt {1-e^{2}}}}{1+e\cos {\theta }}}} cos E = e + c o s θ 1 + e cos θ {\displaystyle \cos {E}={\frac {e+cos{\theta }}{1+e\cos {\theta }}}} E n + 1 = E n + M − E n + e sin E 1 − e cos E {\displaystyle E_{n+1}=E_{n}+{\frac {M-E_{n}+e\sin E}{1-e\cos E}}}
E n + 1 = E n + M + E n − e sinh E e cosh E − 1 {\displaystyle E_{n+1}=E_{n}+{\frac {M+E_{n}-e\sinh E}{e\cosh E-1}}}
θ = cos − 1 ( p r e − 1 e ) {\displaystyle \theta =\cos ^{-1}\left({\frac {p}{re}}-{\frac {1}{e}}\right)}
cos ϕ = 1 − e 2 1 − e 2 cos 2 E {\displaystyle \cos \phi ={\sqrt {\frac {1-e^{2}}{1-e^{2}\cos ^{2}E}}}}
cos ϕ = e 2 − 1 e 2 cosh 2 E − 1 {\displaystyle \cos \phi ={\sqrt {\frac {e^{2}-1}{e^{2}\cosh ^{2}E-1}}}}