Determining work of a 3 particle system

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SUMMARY

The discussion focuses on calculating the height a particle reaches when launched from the surface of a spherical asteroid with a radius of 500 km and a gravitational acceleration of 3.0 m/s². The participant initially used conservation of energy principles but arrived at an incorrect height of 166,666.67 meters above the surface. The correct calculation, which involves using the gravitational potential energy formula U=-(GmM)/r, yields a height of 250,000 meters above the surface. The participant acknowledges the need to adjust their approach due to varying gravitational conditions.

PREREQUISITES
  • Understanding of gravitational potential energy (U=-(GmM)/r)
  • Familiarity with conservation of energy principles (Ui + ki = Uf + kf)
  • Basic knowledge of kinematics and dynamics (f=ma)
  • Ability to manipulate equations involving gravitational forces and accelerations
NEXT STEPS
  • Study the application of conservation of energy in non-uniform gravitational fields
  • Learn about gravitational potential energy calculations for celestial bodies
  • Explore the implications of varying gravitational acceleration on projectile motion
  • Investigate the mass and density calculations for asteroids and their effects on gravitational forces
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitational systems, as well as educators seeking to clarify concepts related to energy conservation in celestial contexts.

Dusty912
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Homework Statement


on a spherical astroid with a radius of 500km and an acceleration due to gravity of 3.0m/s2
How far from the surface will a particle go if it leaves the asteroid’s surface with a radial speed of 1000m/s?

Homework Equations


conservation of energy
Ui + ki=Uf +kf
U=-(GmM)/r
K=(1/2)mv2
-------------------------
f=ma
-(GmM)/r2=ma
-(GM)/r2=a
-(GM)/r=ar
(can apply to h height)

r=radius of astroid
h=height above center
m=mass of rocket
M=mass of astroid
G=gravitational constant
a=acceleration due to asteroids gravity

The Attempt at a Solution


Ui + ki=Uf +kf
Ui + ki=Uf + 0
-(GmM)/r +(1/2)mvi2=-(GmM)/h
the m masses cancel
-(GM)/r +(1/2)vi2=-(GM)/h
-ar +(1/2)vi2=-ah
r-(1/2)(1/a)vi2=h
plugging in the values gives me
500000m+(1/2)(1/(3m/s2)(1000m/s2)2=h

5166666.667meters from the center of the astroid. so 166666.667 meters above its surface. Which is the incorrect answer. the right answer is 250000 meters above the surface.

I know this should be a pretty simple problem, Not too sure where I went wrong. Thanks ahead of time
 
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Okay so I realized that I cannot use mgh fro the U final because the acceleration due to gravity is different here. So I found the mass of the astroid. If I use U=-(GmM)/r and solve for h will I get the correct answer?

and btw the title is wrong for this post.
 

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