Final answer:
The centripetal acceleration of a geosynchronous satellite can be calculated using the formula ac = (4π²r) / T², where r is the distance from the center of the satellite to the center of Earth and T is the period of the satellite. Plugging in the given values, the centripetal acceleration is approximately 0.0056 m/s².
Step-by-step explanation:
The centripetal acceleration of a satellite can be calculated using the formula:
ac = (4π²r) / T²
where ac is the centripetal acceleration, r is the distance from the center of the satellite to the center of Earth, and T is the period of the satellite.
Plugging in the given values:
ac = (4π² times 42,250,000) / (24 times 3600)²
Simplifying, we get:
ac ≈ 0.0056 m/s²
Therefore, the centripetal acceleration of the geosynchronous satellite is approximately 0.0056 m/s², which corresponds to option b).