Gravitational Forces and Motion in a System of Four Bodies

AI Thread Summary
The discussion focuses on calculating gravitational forces and motion involving three fixed spheres and a small particle. For part (a), the force on the 0.0250-kg particle at point P was determined to be approximately 1.11875e-11 N at a 45-degree angle. In part (b), the challenge lies in finding the particle's speed as it moves from a position 300 m away from the origin. Participants suggest using conservation principles and calculating the change in gravitational potential energy to solve for the speed. The conversation emphasizes the need to consider vector forces and the distances from the particle to each mass for accurate calculations.
whiteway
Messages
7
Reaction score
0

Homework Statement


Three uniform spheres are fixed at the positions shown in the figure below. (m1 = 1.0 kg, m2 = 2.0 kg, and d = 0.60 m.)

(See attached picture)

(a) What are the magnitude and direction of the force on a 0.0250-kg particle placed at P?


(b)If the spheres are in deep outer space and a 0.0250-kg particle is released from rest 300 m from the origin along a line 45° below the -x-axis, what will the particle's speed be when it reaches the origin?


Homework Equations



I used some good old trig and GMm/r^2 to get the answers to a, which were 1.11875e-11 N and 45 degrees.

for b I really have no idea where to go with it...



The Attempt at a Solution

 

Attachments

  • 12-40alt.gif
    12-40alt.gif
    1.5 KB · Views: 645
Physics news on Phys.org
whiteway said:
for b I really have no idea where to go with it...
Hint: What's conserved?
 
hmm...
Do I need to break the problem into vector forces with GMm/r from p to each mass and find the total force by adding those?
 
whiteway said:
hmm...
Do I need to break the problem into vector forces with GMm/r from p to each mass and find the total force by adding those?
For b you need to find the speed of the particle after it moves from its initial position (how far is that position from each mass?) to its final position at point P. Hint: Calculate the change in gravitational potential energy as it moves.
 
I multiplied the values first without the error limit. Got 19.38. rounded it off to 2 significant figures since the given data has 2 significant figures. So = 19. For error I used the above formula. It comes out about 1.48. Now my question is. Should I write the answer as 19±1.5 (rounding 1.48 to 2 significant figures) OR should I write it as 19±1. So in short, should the error have same number of significant figures as the mean value or should it have the same number of decimal places as...
Thread 'A cylinder connected to a hanging mass'
Let's declare that for the cylinder, mass = M = 10 kg Radius = R = 4 m For the wall and the floor, Friction coeff = ##\mu## = 0.5 For the hanging mass, mass = m = 11 kg First, we divide the force according to their respective plane (x and y thing, correct me if I'm wrong) and according to which, cylinder or the hanging mass, they're working on. Force on the hanging mass $$mg - T = ma$$ Force(Cylinder) on y $$N_f + f_w - Mg = 0$$ Force(Cylinder) on x $$T + f_f - N_w = Ma$$ There's also...
Back
Top