https://en.wikipedia.org/wiki/Centripetal_force#General_planar_motionDr. Surgery said:How can you calculate centripetal acceleration in a non circular system(I.E. if wanted to calculate the centripetal acceleration in an eclipse, or a parabola how could I do that?)
Centripetal acceleration is the acceleration experienced by an object moving in a circular path. It is always directed towards the center of the circle and its magnitude depends on the object's speed and the radius of the circle.
Normal acceleration is the acceleration experienced by an object in a straight line. Centripetal acceleration, on the other hand, is the acceleration experienced by an object moving in a circular path. It is always perpendicular to the object's velocity and directed towards the center of the circle.
The formula for calculating centripetal acceleration is a = v²/r, where "a" is the centripetal acceleration, "v" is the velocity of the object, and "r" is the radius of the circle.
Centripetal acceleration causes an object to continuously change its direction, or velocity, as it moves in a circular path. This acceleration is necessary to keep the object from traveling in a straight line and maintaining its circular motion.
Some examples of centripetal acceleration in our daily lives include the motion of a car around a curve, the rotation of a Ferris wheel, and the orbit of planets around the sun. Any object moving in a circular path experiences centripetal acceleration.