Retarded Force in Space and interstellar dust

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SUMMARY

The discussion focuses on calculating the retarding force acting on a uniform, spherical planet of mass M and radius R as it moves slowly through a cloud of interstellar dust with density ρ. Key equations utilized include conservation of momentum (Li = Lf), conservation of energy, and the potential energy formula (GMm/R²). The solution involves expressing the retarding force in terms of the planet's speed v, radius R, mass M, and the density of the dust ρ, emphasizing the importance of the equation F = dP/dt for determining the force.

PREREQUISITES
  • Understanding of conservation laws in physics, specifically momentum and energy.
  • Familiarity with gravitational potential energy calculations (GMm/R²).
  • Knowledge of basic kinematics and dynamics, particularly relating to forces.
  • Ability to manipulate equations involving mass, density, and velocity.
NEXT STEPS
  • Study the application of conservation of momentum in non-collisional systems.
  • Learn about gravitational interactions in astrophysics, focusing on dust and planetary formation.
  • Explore the implications of retarding forces in celestial mechanics.
  • Investigate the relationship between density and gravitational attraction in astrophysical contexts.
USEFUL FOR

This discussion is beneficial for physics students, astrophysicists, and anyone interested in celestial mechanics and the dynamics of planetary motion through interstellar media.

whiztle
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Homework Statement


A uniform, spherical planet of mass M and radius R moves SLOWLY with an essentially uniform speed v through a cloud of interstellar dust particles, whose density is ρ. The dust particles are attracted towards the planet, and some of them would eventually fall onto its surface.

Find the resulting retarding force on the planet due to the dust cloud.?
Since the planet moves slowly, initial speed and final speed can be assumed to be the same

Homework Equations


Angular momentum => Li = Lf
Momentum => Pi = Pf
Energy including
Potential energy = GMm/R2
Kinetic Energy = 1/2 (mv2)

The Attempt at a Solution



The clue is to use conservation of momentum, angular momentum, and energy.
Solution should be in terms of speed v, radius R, mass M, and density ρ.
 
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Hmm... well, the clue you give suggests that maybe this isn't what is intended, but are you familiar with this equation?
F = \frac{\mathrm{d}p}{\mathrm{d}t}
That's my first thought...
 

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