Cosmic Calculations and Kinetic Energy

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SUMMARY

The discussion focuses on calculating gravitational potential energy changes and kinetic energy for a satellite moving between two orbits around Earth. The satellite, with a mass of 500 kg, transitions from an orbit with a radius of 2 Earth radii to one with a radius of 3 Earth radii. Key calculations include the initial potential energy (Epi) of -1.5637 x 10^10 J, the final potential energy (Epf) of -1.042 x 10^10 J, and a change in potential energy of 5.20 x 10^9 J. The required orbital speed for the new orbit is calculated to be 4566 m/s, and the escape velocity from Earth's surface is determined to be approximately 11184.48 m/s.

PREREQUISITES
  • Understanding of gravitational potential energy equations, specifically E_p = -G(m_1*m_2)/r
  • Familiarity with the concept of circular orbits and orbital mechanics
  • Knowledge of escape velocity calculations, v_escape = sqrt((2*G*m_planet)/r)
  • Basic proficiency in algebra and square root calculations
NEXT STEPS
  • Study the implications of energy conservation in orbital mechanics
  • Learn about the effects of varying orbital radii on satellite speed and energy
  • Explore the concept of work done by conservative forces in gravitational fields
  • Investigate the relationship between kinetic energy and potential energy in satellite motion
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and gravitational forces, as well as educators looking for practical examples of orbital calculations.

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Homework Statement



A satellite with a mass of 5.00 x 10^2kg is in a circular orbit, whose radius is 2(radius of the earth), around earth. Then it is moved to a circular orbit with a radius of 3(radius of the earth).

a) Determine the satellite's gravitational potential energy from the first orbit to the second orbit.
b) Determine the change in gravitational potential energy from the first orbit to the second orbit.
c) Determine the work done in moving the satellite from the first orbit to the second orbit. Apply energy conservation.
d) Calculate the speed it would need in order to maintain its new orbit.
e) Calculate the escape velocity for the satellite if it is on the Earth's surface.

mass of Earth : 5.98 x 10^24 kg
radius of the Earth : 6.38 x 10^6 m

Homework Equations


E_p = -1(G*m_1*m_2)/r
(delta)E_p = -((G*m_1*m_2)/r) - (-((G*m_1*m_2)/r))
v = sqrt((G*m_planet)/r)
v_escape = sqrt((2*G*m_planet)/r)



The Attempt at a Solution



a) Epi=[(-G)(5.98x10^24kg)(5.00x10^2kg)]/2(6.38x10^6m)
Epi=-1.5637x1010J

Epf=[(-G)(5.98x10^24kg)(5.00x10^2kg)]/3(6.38x10^6m)
Epf=-1.042x10^10J

b)

Change in Ep= Epf-Epi
Change in Ep= (-1.042x10^10J)-(-1.5637x1010J)
Change in Ep=5.20x10^9J

c)

This is where I'm having trouble, in this case does Changes in Ep= Work ?
Or is Change in Ep+ Ek = Work ?

d)

v=Sqr[ [(G)(5.98x10^24kg)]/3(6.38x10^6m)]
v=4566m/s

e)

Vesp = Sqr [ [(2G)(5.98x10^24 kg)] / (6.38x10^6m) ]
Vesp =111.84.48 m/s

Could some verify my solutions, and shed some light on my problems in c)
 
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work is simply the change in potential energy, so final PE - initial PE, which should work out to be a positive value
 
hy23 is right ...

and more precisely ...

W(internel conservative forces) = -(Uf - Ui) = Ui - Uf

dont think that work can only be positive ... negative work do exist!
 
yes negative work do exist, I meant in his case, since he's going from a very negative potential energy to a not so negative PE, positive W is done
 

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