Net Gravitational Force on Object #1 with Distances A and B

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SUMMARY

The magnitude of the gravitational force on object #1 due to object #2 is calculated using the formula Fg = Gm1m2/r^2, where G is the gravitational constant (6.67E-11 N(m/kg)^2). The distances involved are A = 0.383 m and B = 0.271 m. The initial calculation provided was correct for the force between object #1 and object #2, but the discussion highlights the need to consider the net gravitational force on object #1, which may also involve the influence of object #3.

PREREQUISITES
  • Understanding of Newton's Law of Universal Gravitation
  • Familiarity with gravitational constant (G)
  • Basic algebra for manipulating equations
  • Knowledge of vector addition for net force calculations
NEXT STEPS
  • Calculate the net gravitational force on object #1 considering all influencing objects.
  • Review vector addition techniques for combining forces in physics.
  • Explore the implications of multiple gravitational forces acting on a single object.
  • Study gravitational force calculations in different configurations and distances.
USEFUL FOR

Students studying physics, particularly those focused on gravitational forces and their calculations, as well as educators looking for examples of gravitational interactions in problem-solving contexts.

madasrabbits
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Homework Statement


What is the magnitude of the gravitational force on object #1 as a result of object #2? Distance A = 0.383 m and distance B = 0.271 m.
the diagram for the problem is here:
http://students.physicsygoodness.com/user/1/graphics/image001.gif

Homework Equations



Fg= Gm1m2/r^2

The Attempt at a Solution


I tried simply plugging in the masses and using the distance for the radius.
Fg= (6.67E+-11)(10)(10)/(.383)^2
I don't know if object #2 is impacted by the gravitational force of object #3...I don't know how to incorporate that
 
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madasrabbits said:

Homework Statement


What is the magnitude of the gravitational force on object #1 as a result of object #2? Distance A = 0.383 m and distance B = 0.271 m.
the diagram for the problem is here:
http://students.physicsygoodness.com/user/1/graphics/image001.gif

Homework Equations



Fg= Gm1m2/r^2

The Attempt at a Solution


I tried simply plugging in the masses and using the distance for the radius.
Fg= (6.67E+-11)(10)(10)/(.383)^2
I don't know if object #2 is impacted by the gravitational force of object #3...I don't know how to incorporate that

I would say that you've answered the question correctly, namely "What is the magnitude of the gravitational force on object #1 as a result of object #2?" You found [itex]\rm ||{\bf F}_{21}|| = \frac{Gm_1m_2}{r_{12}^2}[/itex] .

Perhaps you should try to find the net force on object #1 now.
 

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