Rocket science

A single-stage rocket is launched vertically from the North Pole and reaches just the required escape velocity to leave the earth after burning its entire fuel.

What is the fuel mass m fuel m_\text{fuel} of the rocket in units of the empty weight m 0 m_0 (rocket without fuel)?

Assumptions:

  • The fuel is consumed with a constant rate m ˙ = const |\dot m| = \text{const} and the combustion gases are expelled with a velocity u 0 = 3 km / s u_0 = 3 \, \text{km} / \text{s} from the nozzle.
  • The gravitational acceleration at the North Pole is g = 9.82 m / s 2 g = 9.82 \, \text{m} / \text{s}^2 and the radial distance to the center of the earth is R = 6350 km R = 6350 \, \text{km} .

Hint: Without external forces, the total momentum of the rocket and the fuel gases must be conserved. The rocket itself changes its momentum p = m v p = m v because of its acceleration v ˙ \dot v , the mass decrease m ˙ \dot m , and the momentum of the ejected gas.

Bonus question: How much fuel would be saved if the rocket were started instead of the North Pole from the equator?

m fuel 10 m 0 m_\text{fuel} \approx 10 m_0 m fuel 20 m 0 m_\text{fuel} \approx 20 m_0 m fuel 5 m 0 m_\text{fuel} \approx 5 m_0 m fuel 40 m 0 m_\text{fuel} \approx 40 m_0 m fuel 80 m 0 m_\text{fuel} \approx 80 m_0

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1 solution

Markus Michelmann
Oct 17, 2017

The momentum balance for the force-free rocket reads d p d t = ( d p d t ) rocket + ( d p d t ) gas = ( m ˙ v + m v ˙ ) m ˙ ( v u 0 ) = m ˙ u 0 + m v ˙ = ! 0 v ˙ = u 0 m ˙ m = u 0 m ˙ m 0 m ˙ ( t t 0 ) \begin{aligned} \frac{dp}{dt} &= \left(\frac{dp}{dt}\right)_\text{rocket} + \left(\frac{dp}{dt}\right)_\text{gas} \\ &= (\dot m v + m \dot v) - \dot m (v - u_0) = \dot m u_0 + m \dot v \stackrel{!}{=} 0 \\ \Rightarrow \quad \dot v &= - u_0 \frac{\dot m}{m} = u_0 \frac{|\dot m|}{m_0 - |\dot m|(t - t_0)} \end{aligned} with the burning time t 0 = m fuel / m ˙ t_0 = m_\text{fuel}/|\dot m| of the rocket. Integration from t = 0 t = 0 to t 0 t_0 results the final velocity v 0 = u 0 0 t 0 d t m 0 / m ˙ + t 0 t = u 0 ln m 0 / m ˙ + t 0 m 0 / m ˙ = u 0 ln m 0 + m fuel m 0 \begin{aligned} v_0 &= u_0 \int_0^{t_0} \frac{ dt}{m_0/|\dot m| + t_0 - t} = u_0 \ln \frac{m_0/|\dot m| + t_0}{m_0/|\dot m|} \\ &= u_0 \ln \frac{m_0 + m_\text{fuel}}{m_0} \end{aligned} The work integral over the gravitational force results the necessary energy to leave the earth: W = R F d r = R G M m 0 r 2 d r = R m 0 g R 2 r 2 d r = m 0 g R = ! 1 2 m 0 v 0 2 v 0 = 2 g R = 11.167 km s m fuel = m 0 ( exp ( v 0 u 0 ) 1 ) 40.37 m 0 \begin{aligned} & & W &= - \int_{R}^{\infty} F dr = \int_R^\infty G \frac{M m_0}{r^2} dr = \int_R^\infty m_0 g \frac{R^2}{r^2} dr = m_0 g R\\ & & &\stackrel{!}{=} \frac{1}{2} m_0 v_0^2 \\ \Rightarrow & & v_0 &= \sqrt{2 g R} = 11.167\,\frac{\text{km}}{s} \\ \Rightarrow & & m_\text{fuel} &= m_0 \left(\exp\left(\frac{v_0}{u_0}\right) - 1\right) \approx 40.37 \cdot m_0 \end{aligned}

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