Cloverleaf exits are approximately circular. A 1220 kg automobile is traveling 56 mph while taking a cloverleaf exit that has a radius of 35.9 m. Calculate the centripetal acceleration of the car and the centripetal force on the car. Remember that 1 mph = 0.447 m/s.

2.A satellite is in orbit about Earth. Its orbital radius is 7.29×107 m. The mass of the satellite is 4362 kg and the mass of Earth is 5.974×1024 kg. Determine the orbital speed of the satellite in mi/s. 1 mi/s = 1609 m/s.

56 miles/ hr * .447 m/s / mile/hr = 25 m/s

Ac = v^2/R = 625 / 35.9 = 17.4 /s^2 (wow, g is only about 9.81)
F = m Ac

again F = m Ac
this time F = G Mearth m/R^2
and m Ac = m v^2/R
so
G Mearth/R^2 = v^2/R
so
v^2 = G Mearth /R

6.67*10^-11 is G

by the way, the mass of a satellite in orbit does not matter. If you set your coffee cup outside the space station it stays alongside in theory. Notice that m cancels.

To calculate the centripetal acceleration of the car, we can use the formula:

a = v^2 / r

where "a" is the centripetal acceleration, "v" is the velocity, and "r" is the radius.

First, we need to convert the velocity from mph to m/s. Since 1 mph = 0.447 m/s:

v = 56 mph * 0.447 m/s = 25.032 m/s

Substituting the values into the formula:

a = (25.032 m/s)^2 / 35.9 m

a = 627.648 m^2/s^2 / 35.9 m

a ≈ 17.50 m/s^2

So, the centripetal acceleration of the car is approximately 17.50 m/s^2.

To calculate the centripetal force on the car, we can use the formula:

F = m * a

where "F" is the centripetal force, "m" is the mass, and "a" is the centripetal acceleration.

Substituting the values into the formula:

F = 1220 kg * 17.50 m/s^2

F ≈ 21,350 N

Therefore, the centripetal force on the car is approximately 21,350 N.

Now, let's move on to the second question.

To determine the orbital speed of the satellite in mi/s, we can use the formula:

v = √(G * (M / r))

where "v" is the orbital speed, "G" is the gravitational constant (approximately 6.67430 × 10^-11 N m^2/kg^2), "M" is the mass of Earth, and "r" is the orbital radius.

First, let's convert the orbital radius from meters to miles:

7.29 × 10^7 m / 1609 m/mi ≈ 45,265 mi

Substituting the values into the formula:

v = √(6.67430 × 10^-11 N m^2/kg^2 * (5.974 × 10^24 kg) / (45,265 mi))

v ≈ √(3.98510 × 10^14 m^3/kg/s^2 * (5.974 × 10^24 kg) / (45,265 mi))

v ≈ √(2.38353 x 10^51 m^3/s^2) ≈ 1.5455 × 10^26 m/s

Now, let's convert the orbital speed from m/s to mi/s:

1.5455 × 10^26 m/s / 1609 m/s/mi ≈ 9.607 × 10^22 mi/s

Therefore, the orbital speed of the satellite is approximately 9.607 × 10^22 mi/s.