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A centripetal force (from Latin centrum, "center" and petere, "to seek" [1]) is a force that makes a body follow a curved path.The direction of the centripetal force is always orthogonal to the motion of the body and towards the fixed point of the instantaneous center of curvature of the path.
This acceleration is known as centripetal acceleration. For a path of radius r , when an angle θ is swept out, the distance traveled on the periphery of the orbit is s = rθ . Therefore, the speed of travel around the orbit is v = r d θ d t = r ω , {\displaystyle v=r{\frac {d\theta }{dt}}=r\omega ,} where the angular rate of rotation is ω .
The radial acceleration (perpendicular to direction of motion) is given by = =. It is directed towards the center of the rotational motion, and is often called the centripetal acceleration . The angular acceleration is caused by the torque , which can have a positive or negative value in accordance with the convention of positive and negative ...
which breaks into the radial acceleration d 2 r / dt 2 , centripetal acceleration –rω 2, Coriolis acceleration 2ω dr / dt , and angular acceleration rα. Special cases of motion described by these equations are summarized qualitatively in the table below.
This orbit has no radial version. Listed below is a circular orbit in astrodynamics or celestial mechanics under standard assumptions. Here the centripetal force is the gravitational force, and the axis mentioned above is the line through the center of the central mass perpendicular to the orbital plane.
are called the tangential acceleration and the normal or radial acceleration (or centripetal acceleration in circular motion, see also circular motion and centripetal force), respectively. Geometrical analysis of three-dimensional space curves, which explains tangent, (principal) normal and binormal, is described by the Frenet–Serret formulas ...
This centripetal acceleration is provided by a centripetal force, which is exerted on the body in curved motion by some other body. In accordance with Newton's third law of motion , the body in curved motion exerts an equal and opposite force on the other body.
Classical mechanics is the branch of physics used to describe the motion of macroscopic objects. [1] It is the most familiar of the theories of physics. The concepts it covers, such as mass, acceleration, and force, are commonly used and known. [2]