Post

Created by @nathanedwards
 at November 4th 2023, 7:11:34 pm.

AP Physics 1 Exam Question - Gravitational Force and Fields

A spacecraft of mass mm is in a circular orbit around a planet of mass MM and radius rr. The spacecraft is moving at a constant speed, which allows it to maintain its circular orbit. The gravitational force between the spacecraft and the planet can be given by the equation:

F=GMmr2F = \frac{G \cdot M \cdot m}{r^2}

Where:

  • FF is the gravitational force between the spacecraft and the planet.
  • GG is the gravitational constant (6.674×10116.674 \times 10^{-11} N m2^2/kg2^2).

a) Derive an expression for the gravitational field strength at a point on the orbit of the spacecraft in terms of MM, rr, and GG.

b) Calculate the gravitational field strength for a spacecraft in a circular orbit around Earth at an altitude of 300 km, assuming a mass of 2×1042 \times 10^4 kg for the spacecraft and a mass of 5.97×10245.97 \times 10^{24} kg for Earth.


Answer:

a) Deriving the expression for gravitational field strength:

The gravitational field strength at a point is defined as the gravitational force experienced by a unit mass placed at that point.

The formula for gravitational field strength, gg, is given by:

g=Fmg = \frac{F}{m}

We can substitute the expression for gravitational force, FF, into the equation above:

g=GMmr2mg = \frac{\frac{G \cdot M \cdot m}{r^2}}{m}

Canceling out the mass mm on both numerator and denominator, we get:

g=GMr2g = \frac{G \cdot M}{r^2}

Hence, the expression for gravitational field strength at a point on the orbit of the spacecraft is:

g=GMr2g = \frac{G \cdot M}{r^2}

b) Calculating the gravitational field strength:

Given:

  • Mass of spacecraft, m=2×104m = 2 \times 10^4 kg
  • Mass of Earth, M=5.97×1024M = 5.97 \times 10^{24} kg
  • Radius, r=6,371r = 6,371 km (radius of Earth + altitude)

First, convert the radius to meters:

r=6,371×1000=6.371×106mr = 6,371 \times 1000 = 6.371 \times 10^6 \, \text{m}

Now, substitute the values into the expression for gravitational field strength:

g=GMr2g = \frac{G \cdot M}{r^2}
g=(6.674×1011N m2/kg2)(5.97×1024kg)(6.371×106m)2g = \frac{(6.674 \times 10^{-11} \, \text{N m}^2/\text{kg}^2) \cdot (5.97 \times 10^{24} \, \text{kg})}{{(6.371 \times 10^6 \, \text{m})}^2}
g=(6.674×1011N m2/kg2)(5.97×1024kg)4.053×1013m2g = \frac{(6.674 \times 10^{-11} \, \text{N m}^2/\text{kg}^2) \cdot (5.97 \times 10^{24} \, \text{kg})}{4.053 \times 10^{13} \, \text{m}^2}
g=3.972×10144.053×1013N/kgg = \frac{3.972 \times 10^{14}}{4.053 \times 10^{13}} \, \text{N/kg}
g9.81N/kgg \approx 9.81 \, \text{N/kg}

Therefore, the gravitational field strength for a spacecraft in a circular orbit around Earth at an altitude of 300 km is approximately 9.81N/kg9.81 \, \text{N/kg}.