Answer: D. 0.57
Step-by-step explanation:
The formula to calculate the eccentricity
of an ellipse is (assuming the moon's orbit in the shape of an ellipse):
![e=(r_(a)-r_(p))/(r_(a)+r_(p))](https://img.qammunity.org/2021/formulas/physics/middle-school/6jv2z368dwv2yc872mwmg7udhmtnh03gnh.png)
Where:
is the apoapsis (the longest distance between the moon and its planet)
is the periapsis (the shortest distance between the moon and its planet)
Then:
![e=(r_(a)-0.27 r_(a))/(r_(a)+0.27 r_(a))](https://img.qammunity.org/2021/formulas/physics/middle-school/3j9rjx3mlghiply9rpj4mb0tnvmzpd19dn.png)
![e=(0.73 r_(a))/(1.27 r_(a))](https://img.qammunity.org/2021/formulas/physics/middle-school/kb2t1pnem2f9x42q8ogoqs650u5j92jpyz.png)
This is the moon's orbital eccentricity