The formula for calculating the circular orbit velocity of an object around a central body is v (GM/r), where v is the velocity, G is the gravitational constant, M is the mass of the central body, and r is the distance between the object and the central body.
The formula for calculating the angular velocity of an object in circular motion is angular velocity () linear velocity (v) / radius of rotation (r).
The formula for calculating the linear velocity (v) of an object in circular motion is v r w, where v is the linear velocity, r is the radius, and w is the angular velocity.
The formula for calculating velocity in a pipe is velocity flow rate / cross-sectional area.
The formula for the velocity of an object in circular orbit around a central body is v (gm/r), where v is the velocity, g is the gravitational constant, m is the mass of the central body, and r is the distance between the object and the center of the central body.
The formula for calculating centripetal acceleration in terms of the radius of the circular motion is a v2/r, where "a" represents the centripetal acceleration, "v" is the velocity of the object in circular motion, and "r" is the radius of the circle.
The formula for calculating the angular velocity of an object in circular motion is angular velocity () linear velocity (v) / radius of rotation (r).
The formula for calculating the linear velocity (v) of an object in circular motion is v r w, where v is the linear velocity, r is the radius, and w is the angular velocity.
The formula for calculating velocity in a pipe is velocity flow rate / cross-sectional area.
The formula for the velocity of an object in circular orbit around a central body is v (gm/r), where v is the velocity, g is the gravitational constant, m is the mass of the central body, and r is the distance between the object and the center of the central body.
The formula for calculating centripetal acceleration in terms of the radius of the circular motion is a v2/r, where "a" represents the centripetal acceleration, "v" is the velocity of the object in circular motion, and "r" is the radius of the circle.
The circular orbit velocity formula is v (GM/r), where v is the velocity, G is the gravitational constant, M is the mass of the central object, and r is the distance from the center. This formula is used in physics to calculate the velocity required for an object to stay in a circular orbit around a central mass, such as a planet or a star. It helps scientists understand the dynamics of celestial bodies and spacecraft in orbit.
The formula for calculating acceleration is: acceleration (final velocity - initial velocity) / time elapsed.
The formula for calculating acceleration is: acceleration change in velocity / time.
The circular orbit formula is used to calculate the speed of an object moving in a circular path. It is expressed as v (GM/r), where v is the velocity of the object, G is the gravitational constant, M is the mass of the central body, and r is the radius of the circular path. This formula helps determine the velocity needed for an object to maintain a stable orbit around a central body, such as a planet or a star.
The change in time formula for calculating the velocity of an object is: velocity (final position - initial position) / (final time - initial time).
The formula for calculating fluid velocity in a pipe is V Q/A, where V is the velocity, Q is the flow rate, and A is the cross-sectional area of the pipe.
The formula for calculating the velocity of longitudinal waves is v (E/), where v is the velocity of the wave, E is the elastic modulus of the material, and is the density of the material.