# Centripetal Acceleration of an Ellipse

• Philosophaie
In summary, the centripetal acceleration of a circle is a_c = \frac{v^2}{r} * u_n. The acceleration of an ellipse increases from apoapsis to periapsis and then decreases from periapsis to apoapsis as the position changes from furthest point in the orbit to the closest and vice versa. To calculate the centripetal acceleration of an ellipse, the central point must be located at a focus of the ellipse and the central force must vary as 1/r^2 where r is the distance from the body to that central point. This is the only way to produce an elliptical path that does not precess. However, a radial harmonic oscillator can also produce an elliptical trajectory,

#### Philosophaie

The centripetal acceleration of a circle is: $$a_c = \frac{v^2}{r} * u_n.$$ The acceleration of an ellipse is different. It increases from from apoapsis to periapsis as the position changes from furthest point in the orbit to the closest. Then decreases from from periapsis to apoapsis as the position changes from closest point to the furthest. Is there a way to calculate this centripetal acceleration of an ellipse due to the change in the normal and the varying of position due to the gravitating body?

Philosophaie said:
The centripetal acceleration of a circle is: $$a_c = \frac{v^2}{r} * u_n.$$ The acceleration of an ellipse is different. It increases from from apoapsis to periapsis as the position changes from furthest point in the orbit to the closest. Then decreases from from periapsis to apoapsis as the position changes from closest point to the furthest. Is there a way to calculate this centripetal acceleration of an ellipse due to the change in the normal and the varying of position due to the gravitating body?
The only way to make a body prescribe an elliptical path due to a centripetal force (ie. a force that is always directed toward a central point whose location does not change) is to have that central point located at a focus of the ellipse and have the central force vary as 1/r^2 where r is the distance from the body to that central point (focus).

So if you know its tangential speed at the perigee or apogee (radial component is 0 so a = v^2/r) you can work out the acceleration at any other point eg.:

$$\frac{a_r}{a_{apogee}} = \frac{r_{apogee}^2}{r^2}$$

AM

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Andrew Mason said:
The only way to make a body prescribe an elliptical path due to a centripetal force (ie. a force that is always directed toward a central point whose location does not change) is to have that central point located at a focus of the ellipse and have the central force vary as 1/r^2 where r is the distance from the body to that central point (focus).
Really? That may be the only sensible way to do it, but I'm pretty sure that given any point whatsoever inside the ellipse, you can produce an elliptical trajectory by a centripetal force that varies appropriately.

Andrew Mason said:
The only way to make a body prescribe an elliptical path due to a centripetal force (ie. a force that is always directed toward a central point whose location does not change) is to have that central point located at a focus of the ellipse and have the central force vary as 1/r^2 where r is the distance from the body to that central point (focus).
Doesn't this redefine "centripetal force"? Using the normal definition, if the only force on an object is centripetal (perpendicular to velocity), then the speed is constant, and only the radius of curvature changes over time. There was a recent thread that worked out the math for an objects traveling at constant speed in an elliptical path.

eigenperson said:
Really? That may be the only sensible way to do it, but I'm pretty sure that given any point whatsoever inside the ellipse, you can produce an elliptical trajectory by a centripetal force that varies appropriately.
Not if you want to produce an elliptical path that keeps repeating itself (ie. an ellipse that does not precess).

You will find that the appropriate variation of the central force to produce a constant elliptical path is a variation of 1/r^2 where r is the distance from the body to the central point. The special case is the circle where there is no variation in r (ie the magnitude of the central force is constant).

The mathematical proof involves finding a very messy solution to a differential equation. Newton figured it out using a geometrical method which is very difficult to follow (See: Feynman's attempt to explain it in "Feynman's Lost Lecture").

AM

rcgldr said:
Doesn't this redefine "centripetal force"? Using the normal definition, if the only force on an object is centripetal (perpendicular to velocity), then the speed is constant, and only the radius of curvature changes over time. There was a recent thread that worked out the math for an objects traveling at constant speed in an elliptical path.
I was assuming that the OP was referring to an object prescribing an elliptical orbit due to a central force - a force that is always pointing toward the same central point. The OP referred to a gravitating body.

If a body's motion is being affected only by a central force, Fc, the acceleration toward that central point (ie. the centripetal acceleration) is simply ac = Fc/m. The centripetal acceleration is perpendicular to velocity only for circular motion or at only two points if the motion is elliptical.

AM

rcgldr said:
Doesn't this redefine "centripetal force"? Using the normal definition, if the only force on an object is centripetal (perpendicular to velocity), then the speed is constant, and only the radius of curvature changes over time. There was a recent thread that worked out the math for an objects traveling at constant speed in an elliptical path.
Centripetal means "toward the center," not "perpendicular to velocity."

• TheGreatEscapegoat
vela said:
Centripetal means "toward the center," not "perpendicular to velocity."
"Centripetal" means "toward the instantaneous center of the path curvature", which is the same as "perpendicular to velocity". See:
http://en.wikipedia.org/wiki/Centripetal_force
Wikipedia said:
Centripetal force (from Latin centrum "center" and petere "to seek") is a force that makes a body follow a curved path: its direction is always orthogonal to the velocity of the body, toward the fixed point of the instantaneous center of curvature of the path.

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I stand corrected. Andrew Mason said:
The only way to make a body prescribe an elliptical path due to a centripetal force (ie. a force that is always directed toward a central point whose location does not change) is to have that central point located at a focus of the ellipse and have the central force vary as 1/r^2 where r is the distance from the body to that central point (focus).

No, this is not the only way. A radial harmonic oscillator, whose force is proportional to r, will also have an elliptic orbit, with the center of revolution in the center of the ellipse, not at a focus. According to Bertrand's theorem, this and the inverse-square law are the only two systems that admit closed orbits, which then happen to be elliptic.

Note that any central attractive force admits a circular orbit.

However, since the original question explicitly involved a "gravitating body", we probably needn't consider anything except the inverse-square law to answer it.

Andrew Mason said:
I was assuming that the OP was referring to an object prescribing an elliptical orbit due to a central force - a force that is always pointing toward the same central point. [..]
Interesting! I see that it's also how Newton used it:
http://gravitee.tripod.com/booki3.htm (simply press "cancel").
the law of the centripetal force tending to the focus of the ellipsis
The Wikipedia article also cites his definition:
A centripetal force is that by which bodies are drawn or impelled, or in any way tend, towards a point as to a centre.

vela said:
I stand corrected. In fact your answer was correct! Centripetal simply means "seeking the center". :tongue2:
It appears that there are two slightly different definitions of "centripetal force"...

harrylin said:
Centripetal simply means "seeking the center".
Yes, but "center" is ambiguous. The most common and general definition that works for every curved path references the instantaneous center of curvature of the path.

To the OP: are you just interested in the force vector on an elliptical orbit, or are you interested in breaking it into components which are parallel and perpendicular to the velocity?

harrylin said:
In fact your answer was correct! Centripetal simply means "seeking the center". :tongue2:
It appears that there are two slightly different definitions of "centripetal force"...

A.T. said:
Yes, but "center" is ambiguous. The most common and general definition that works for every curved path references the instantaneous center of curvature of the path.

AFAIK the usual description of the OP's scenario is a central force (i.e. a force that is always directed towards a fixed point). not "centripetal".

In general, the central force has two components, normal and tangential to the path of the object around the orbit. Since "normal" is a well defined geometrical notion for any curve in space (see http://en.wikipedia.org/wiki/Frenet–Serret_formulas) calling the normal direction "centripetal" doesn't seem to add any value IMO - the central force only acts along the normal direction at two points around the orbit, except in the special case where the orbit is a circle.

AlephZero said:
AFAIK the usual description of the OP's scenario is a central force (i.e. a force that is always directed towards a fixed point). not "centripetal".
Yet that description of gravitation as a central force is not what the OP wants. Just take a look at other threads recently started by the OP. He wants centripetal force, that is, the component of force normal to the velocity vector.

I'll make one last vain attempt to steer Philosophaie away from this concept.

Philosophaie: Centripetal force, the component of force normal to the velocity vector, is not going to help you in your quest to understand orbits. Gravitation is a central force rather than a centripetal force. Learn how to use polar coordinates. Learn about true anomaly, eccentric anomaly, mean anomaly, and the relationships between them.

## 1. What is centripetal acceleration of an ellipse?

The centripetal acceleration of an ellipse is the acceleration experienced by an object moving in a circular path on the surface of an ellipse. It is directed towards the center of the ellipse and its magnitude is given by the equation a = v^2/r, where v is the velocity of the object and r is the radius of the circle at that point.

## 2. How is the centripetal acceleration of an ellipse different from that of a circle?

The centripetal acceleration of an ellipse is different from that of a circle because the radius of the circle is constant, while the radius of an ellipse changes at different points along its path. Therefore, the magnitude and direction of the centripetal acceleration also changes along the ellipse.

## 3. What factors affect the centripetal acceleration of an ellipse?

The centripetal acceleration of an ellipse is affected by the velocity of the object, the radius of the ellipse, and the mass of the object. In addition, the eccentricity of the ellipse (how elongated it is) also plays a role in determining the magnitude and direction of the acceleration.

## 4. How is the centripetal acceleration of an ellipse calculated?

The centripetal acceleration of an ellipse can be calculated using the equation a = v^2/r, where v is the velocity of the object and r is the radius of the circle at that point. However, since the radius of an ellipse is constantly changing, the acceleration must be calculated at different points along the ellipse and then combined using vector addition.

## 5. What are some real-world applications of centripetal acceleration of an ellipse?

The centripetal acceleration of an ellipse is seen in a variety of real-world applications, such as the motion of planets around the sun, the motion of satellites in orbit, and the motion of roller coasters and other amusement park rides. It is also important in understanding the behavior of objects moving in curved paths, such as cars on a banked track.