High School Derivation for Aphelion and Perihelion Distances

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The formulas for perihelion and aphelion distances in an orbit are derived from the definitions of semi-major axis (SMA) and eccentricity. The perihelion distance is given by a(1-e) and the aphelion distance by a(1+e). This relationship stems from the definition of eccentricity, where the focal points of an ellipse are located at a distance of ±ea from the center. The sum of the distances from any point on the ellipse to the two foci equals 2a. Understanding these concepts is essential for grasping the derivation of these distances.
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I know the formulas for perihelion and aphelion distances in an orbit with SMA a and eccentricity e are a(1-e) and a(1+e), respectively. However, why is this? I can't seem to find any derivations for this anywhere and also cannot figure this out myself.
 
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Not sure what you mean by "why" here. The focus-directrix definition of an ellipse gives you this more or less instantly, but you may have to work harder with other definitions. Or are you trying to prove it from ##F=GMm/r^2##?

Basically, you have told us where you want to go but not where you are. That makes it tricky to give directions.
 
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See any classical mechanics textbook
 
bruhh said:
I know the formulas for perihelion and aphelion distances in an orbit with SMA a and eccentricity e are a(1-e) and a(1+e), respectively. However, why is this? I can't seem to find any derivations for this anywhere and also cannot figure this out myself.
It follows from the definition of the eccentricity: the focal points of an ellipse are at a distance ## \pm e a ## from the center. And for perihelion and aphelion, as for any points on the ellipse, the sum of the distances to the foci must be ## 2a ##.
 
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