Calculate Proton Speed for Earth Magnetic Equator - Magnetism Question 2

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SUMMARY

The discussion focuses on calculating the speed required for a proton to orbit Earth at an altitude of 1670 km above the magnetic equator, where the magnetic field intensity is 4.1 × 10-8 T. The relevant equations include the Lorentz force equation (f1 = qvbsin(theta)), centripetal force (f2 = mv2/(d+R)), and gravitational force (f3 = Gmprotonmearth/(d+R)2). The correct approach involves equating the gravitational force to the centripetal force to solve for the proton's speed (v).

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  • Understanding of Lorentz force and magnetic fields
  • Knowledge of centripetal force and gravitational force equations
  • Familiarity with the mass of a proton and gravitational constant (G)
  • Basic algebra for solving equations
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  • Explore centripetal motion and its applications in orbital mechanics
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Homework Statement



What speed would a proton need to achieve
in order to circle Earth 1670 km above the
magnetic equator, where the Earth’s mag-
netic field is directed on a line between mag-
netic north and south and has an intensity of
4.1 × 10−8 T?
The mass of a proton is 1.673 × 10−27 kg.
Answer in units of m/s.

Homework Equations



f1=qvbsin(theta)
f2=mv^2/(d+R)
f3=Gm(proton)m(earth)/(d+R)^2 where d is 1670 km, and R is Earth distance


The Attempt at a Solution



I tried doing f1+f2=f3, b ut I am not sure if this is right and i don't know how to solve for v
 
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I think you'd want to equate f2 to f3 as the gravitational force of attraction will provide the centripetal force.
 

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