What is centripetal and centrifugal force with examples

'v' is the tangential velocity of the object (while performing circular motion) 'r' is the distance between the center of the rotation and the object.For instance, the gravitational force of the sun is a centripetal force that keeps the earth orbiting around it.Centrifugal forces are fictitious forces that arise when you're in a rotating frame of reference.Its direction is always orthogonal to the motion of the body and towards the fixed point of the instantaneous center of curvature of the path.The centripetal force formula is given as the product of mass (in kg) and tangential velocity (in meters per second) squared, divided by the radius (in meters).The centripetal force acts on objects moving towards circular motion.

'm' is the mass of the object.When no force is acting on an object, it moves in a straight line at constant speed, or stands still.F c = mv2 r m v 2 r.Spinning a ball on string.Where, f is the centripetal force, m is the.The formula to calculate centrifugal force is defined as the negative ratio of the product of mass (in kg) and square of the velocity of the object (in meter per second) to the radius of the circular path ( in meters) in which it is moving.

If a car is rounding a bend, for example, the centripetal force making it move in a curve rather than a straight line is directed along the radius of the circle the car is tracing out.Centripetal and centrifugal forces are the forces experienced by rotating objects.Planets revolving around the sun.That tension is centripetal force.