Final answer:
The acceleration due to gravity at a point on the satellite's orbit is approximately 8.28 m/s^2.
Step-by-step explanation:
To find the acceleration due to gravity at a point on the satellite's orbit, we can use the formula for centripetal acceleration:
ac = v2/r
where ac is the centripetal acceleration, v is the linear velocity of the satellite, and r is the distance from the satellite to the center of the Earth.
We know that the satellite completes one revolution in 105 minutes, so the period T is 105 minutes or 6300 seconds. The linear velocity v can be calculated as the circumference of the orbit divided by the period:
v = 2πr/T
Substituting this value of v into the formula for centripetal acceleration gives:
ac = (2πr/T)2/r
Using the given values of r = 730 km (which is equal to 7.3 x 105 m) and T = 105 minutes (which is equal to 6.3 x 103 s), we can calculate the acceleration due to gravity at a point on the orbit.
Calculating this gives:
ac = (2π(7.3 x 105)/(6.3 x 103))2/(7.3 x 105)
ac ≈ 8.28 m/s2