Gravitational field strength calculation

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SUMMARY

The discussion clarifies the application of two equations for calculating gravitational field strength: g = F/m and g = GM/r². The equation g = F/m is utilized to determine the gravitational force acting on a mass in a gravitational field, while g = GM/r² calculates the gravitational field strength at a distance r from a mass M. The relationship between these equations is established, emphasizing that g = GM/r² is a specific case of g = F/m when considering the gravitational force exerted by a point mass or a spherically symmetric mass distribution.

PREREQUISITES
  • Understanding of Newton's Law of Universal Gravitation
  • Familiarity with the concepts of gravitational force and field strength
  • Basic knowledge of mathematical equations involving force and mass
  • Awareness of the distinction between point masses and spherically symmetric mass distributions
NEXT STEPS
  • Study the derivation of gravitational force equations in classical mechanics
  • Explore the implications of gravitational field strength variations with distance
  • Learn about gravitational field strength calculations for different celestial bodies
  • Investigate the relationship between gravitational fields and electric fields, particularly E = Felectric/q
USEFUL FOR

Students of physics, educators teaching gravitational concepts, and professionals in fields related to astrophysics or engineering who require a solid understanding of gravitational field calculations.

Hannah7h
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In what scenarios would you use the equation g= F/m instead of g=GM/r2 (or vice versa), for calculating gravitational field strength?

Update: is g=F/m used to find the force acting on a mass in a gravitational field (of strength g), whereas g=GM/r2 used to calculate the gravitational field strength at a point in the field created by the object of mass M
 
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g = F/m defines the strength of the gravitational field at any location, in terms of the gravitational force F that acts on a test-mass m placed at that location. (Note that we use a similar definition for electric field: E = Felectric/q.)

g = GM/r2 is an application of that definition to the special case of the gravitational field at a distance r from a point mass, or outside a spherically symmetric mass distribution, at a distance r from the center: $$g = \frac F m = \frac {\left( \frac {GMm} {r^2} \right)} m = \frac {GM} {r^2}$$
 
jtbell said:
g = F/m defines the strength of the gravitational field at any location, in terms of the gravitational force F that acts on a test-mass m placed at that location. (Note that we use a similar definition for electric field: E = Felectric/q.)

g = GM/r2 is an application of that definition to the special case of the gravitational field at a distance r from a point mass, or outside a spherically symmetric mass distribution, at a distance r from the center: $$g = \frac F m = \frac {\left( \frac {GMm} {r^2} \right)} m = \frac {GM} {r^2}$$

Ahh I see that makes sense, thank you
 
Maybe this is what you are asking since you are using lower case g... The gravitational force on a test mass m at a distance r from the center of the Earth is given by GmM/r2, where M is the mass of the earth. At the Earth's surface, the force is given by GmM/R2, where R is the radius of the earth. For small distances from the surface, this equation still holds well and we use g = GM/R2 for the acceleration due to gravity near the Earth's surface, in which case F=mg.

At appreciable distances from the Earth's surface, we have to use r instead of R, hence the other equation.
 

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