The centripetal force F1, the centripetal acceleration A1, the linear velocity V1 and the angular velocity W1 of the object on the earth's equator in circular motion with the rotation of the earth; The centripetal force of the geostationary satellite is F2, the centripetal acceleration is A2, and the angular velocity is W2. Suppose that the mass of the object and the satellite is equal, then a, F1 > F2 B, A1 > A2 C, V1 < V2 D, W1 = W2

The centripetal force F1, the centripetal acceleration A1, the linear velocity V1 and the angular velocity W1 of the object on the earth's equator in circular motion with the rotation of the earth; The centripetal force of the geostationary satellite is F2, the centripetal acceleration is A2, and the angular velocity is W2. Suppose that the mass of the object and the satellite is equal, then a, F1 > F2 B, A1 > A2 C, V1 < V2 D, W1 = W2

Both the object and the synchronous satellite are relatively geostationary, and their angular velocities are equal, ω 1 = ω 2,
According to v = ω R, the orbit radius of the synchronous satellite is large, so V1 < v2
According to a = ω & #178; R, A1 < A2
According to f = ma, F1 < F2
The CD is correct