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Fifty years ago the Apollo 13 mission to the Moon captured the public's imagination when technical issues led to the aborting of the planned Moon landing - Leaving Cert Physics - Question a - 2020

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Fifty years ago the Apollo 13 mission to the Moon captured the public's imagination when technical issues led to the aborting of the planned Moon landing. The three ... show full transcript

Worked Solution & Example Answer:Fifty years ago the Apollo 13 mission to the Moon captured the public's imagination when technical issues led to the aborting of the planned Moon landing - Leaving Cert Physics - Question a - 2020

Step 1

Derive an expression for the period of orbit T of the Moon when it has a radius of orbit R around the Earth (of mass M).

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Answer

To derive the period of orbit, we start with Newton's law of universal gravitation and the formula for centripetal force. The gravitational force providing the necessary centripetal force can be expressed as:

F=GMmR2F = \frac{GMm}{R^2}

Where:

  • G is the gravitational constant,
  • M is the mass of the Earth,
  • m is the mass of the Moon,
  • R is the distance from the center of the Earth to the Moon.

Centripetal force is given by:

F=mv2RF = \frac{mv^2}{R}

Setting these two expressions equal:

GMmR2=mv2R\frac{GMm}{R^2} = \frac{mv^2}{R}

By cancelling out the mass of the Moon and rearranging, we can express v in terms of G, M, and R:

v2=GMRv^2 = \frac{GM}{R}

The period T can be related to the speed v and the radius R by:

T=2πRvT = \frac{2\pi R}{v}

Substituting the expression for v gives:

T=2πRRGMT = 2\pi R \sqrt{\frac{R}{GM}}

Thus, the derived expression for the period of orbit T is:

T=2πR3GMT = 2\pi\sqrt{\frac{R^3}{GM}}

Step 2

Calculate the period of the Moon as it orbits the Earth.

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Answer

Given:

  • Mass of Earth, M=6.0×1024 kgM = 6.0 \times 10^{24} \text{ kg}
  • Radius of the Moon’s orbit, R=3.85×108 mR = 3.85 \times 10^{8} \text{ m}
  • Gravitational constant, G=6.674×1011 m3 kg1 s2G = 6.674 \times 10^{-11} \text{ m}^3\text{ kg}^{-1}\text{ s}^{-2}

Using the derived formula:

T=2πR3GMT = 2\pi\sqrt{\frac{R^3}{GM}}

Substituting the values:

T=2π(3.85×108)3(6.674×1011)(6.0×1024)T = 2\pi\sqrt{\frac{(3.85 \times 10^8)^3}{(6.674 \times 10^{-11})(6.0 \times 10^{24})}}

Calculating:

T=2π5.7309×10254.0044×1014T = 2\pi\sqrt{\frac{5.7309 \times 10^{25}}{4.0044 \times 10^{14}}}

T2.37×106 seconds27.5 daysT \approx 2.37 \times 10^6 \text{ seconds} \approx 27.5 \text{ days}

Step 3

Calculate the gravitational force exerted by the Moon on an astronaut of mass 80 kg when he is 250 km above the surface of the Moon.

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Answer

First, calculate the distance from the center of the Moon:

  • Radius of the Moon: Rmoon=1740 km=1.74×106 mR_{moon} = 1740 \text{ km} = 1.74 \times 10^6 \text{ m}
  • Height above the surface: h=250 km=2.5×105 mh = 250 \text{ km} = 2.5 \times 10^5 \text{ m}
  • Total distance from the center: R=Rmoon+h=1.74×106+2.5×105=1.99×106 mR = R_{moon} + h = 1.74 \times 10^6 + 2.5 \times 10^5 = 1.99 \times 10^6 \text{ m}

Using Newton's law of gravitation:

F=GmMmoonR2F = \frac{GmM_{moon}}{R^2} Where Mmoon=7.3×1022kgM_{moon} = 7.3 \times 10^{22} \text{kg}:

F=(6.674×1011)(80)(7.3×1022)(1.99×106)2F = \frac{(6.674 \times 10^{-11})(80)(7.3 \times 10^{22})}{(1.99 \times 10^6)^2}

Calculating:

F78.73 NF \approx 78.73 \text{ N}

Step 4

Astronauts appear to be weightless when they orbit the Moon. Explain why.

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Answer

Astronauts experience weightlessness when they orbit the Moon due to free-fall conditions. Both the astronaut and the spaceship are in free fall towards the Moon, falling along the same path as the Moon's curvature. Although gravity is still acting on them, they are moving forward fast enough such that the curve of their path matches the curvature of the Moon.

This creates a scenario where the astronauts do not exert a normal force on the spaceship, leading to the sensation of weightlessness. It is important to note that weightlessness does not mean the absence of gravitational force; rather, it indicates that there is no net force acting on the astronauts in the context of their motion.

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