Gravitational field strength problem- help needed

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SUMMARY

The discussion focuses on calculating the gravitational pull of the Moon on the Earth's oceans, which is approximately 3 millionths of the gravitational pull of the Earth on its oceans. Key values include the Moon's radius of 1740 km, mass of 7.35 x 1022 kg, and a gravitational field strength of 1.62 Nkg-1. The gravitational constant G is specified as 6.67 x 10-11 Nm2kg-2. The user attempts to apply the formula g = GM/r2 to derive the gravitational field strength at Earth's surface due to the Moon.

PREREQUISITES
  • Understanding of gravitational field strength calculations
  • Familiarity with the gravitational constant (G)
  • Knowledge of the formula g = GM/r2
  • Basic algebra for manipulating equations
NEXT STEPS
  • Calculate the gravitational field strength at Earth's surface due to the Moon's mass
  • Learn how to derive ratios of gravitational forces using g = GM/r2
  • Explore the impact of the Moon's gravitational pull on ocean tides
  • Investigate the relationship between gravitational field strength and distance from the mass
USEFUL FOR

Students studying physics, particularly those focusing on gravitational forces and their effects, as well as educators seeking to explain the relationship between celestial bodies and ocean tides.

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gravitational field strength problem-urgent help needed

Homework Statement


Moon has a radius of 1740km, Mass of 7.35 x10^ 22kg, grav field strength of moon= 1.62Nkg^-1, distance from Earth to Moon is 380000km G=6.67x10^-11Nm^2kg^-2

The Moon's gravitational pull on the Earth causes the ocean tides. Show that the gravitational pull of the Moon on the Earth's oceans is approximately 3 millionths of the gravitational pull of the Earth on its oceans.


Homework Equations


g = GM / r^2 g = gs R^2 / r^2 where R= radius of planet, r = distance

The Attempt at a Solution


g = gs R^2 / r^2
1.62 = gs 1740x10^3 / 380000 x 10^3
(1.62 x 380000x10^3) / 1740 x 10^3 = gs

1/3000000= 3 x10^-6
3 x10^-6 x 9.81 = gs ?
Please help!
 
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I don't think you've done it quite right, but you're not far off. You equations are a little confusing also.

I would first try to calculate the gravitational field at Earth due to the mass of the moon (as an equation). And then calculate the gravitational field at Earth's surface due to the mass of the Earth (as another equation). Then divide one by the other to get the ratio.
 

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