Exam review question about space shuttle orbits at differing radii

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SUMMARY

The discussion focuses on calculating the radius of a new orbit for the space shuttle, which makes one revolution every 24 hours, compared to its current orbit at 200 km above Earth's surface with a 1.5-hour period. The key equations involved are the centripetal force equation and the relationship between period and radius, specifically that the period T is proportional to R². The solution involves using the formula R₂ = R₁√(T₂/T₁) to determine the new radius based on the change in orbital period.

PREREQUISITES
  • Understanding of centripetal force and gravitational force balance
  • Familiarity with orbital mechanics and Kepler's laws
  • Knowledge of the formula for tangential velocity v = (2πR)/T
  • Basic algebra for manipulating equations
NEXT STEPS
  • Study the relationship between orbital period and radius in circular orbits
  • Learn about gravitational acceleration and its role in orbital mechanics
  • Explore Kepler's laws of planetary motion for deeper insights
  • Investigate the implications of changing orbital altitudes on satellite operations
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Students studying physics, particularly those focusing on mechanics and orbital dynamics, as well as educators looking for practical examples of gravitational concepts in action.

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Homework Statement



The space shuttle makes 1 revolution around the Earth in 1.5 hours when it is in an orbit 200 km above the Earth’s surface. The radius of the Earth Re is 6.5 × 10^6m. If the shuttle moves to a new orbit such that it makes 1 revolution per day (24 hours), what is the radius of the new orbit?

(1) 6.2Re (2) 12Re (3) 24.8Re (4) 16Re (5) 0.38Re

Homework Equations



Force_centripetal=Force_gravity

v=(2piR)/T

T=period

The Attempt at a Solution



My professor said:

"Yes, the centripetal force is provided by gravity. The tangential velocity v=2piR/T where T is the period. Thus show that T is proportional to R^2 and solve. For orbit 2, R_2=R_1sqrt(T_2/T_1)"

...but I still can't understand what he's talking about. What does he mean that period T is proprtional to r^2? And what does any of this have to do with balancing the centripetal force with the force of gravity?

Thank you. This forum is the best.
 
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hi npersons274! welcome to pf! :smile:

(try using the X2 and X2 buttons just above the Reply box :wink:)
npersons274 said:
"Yes, the centripetal force is provided by gravity. The tangential velocity v=2piR/T where T is the period. Thus show that T is proportional to R^2 and solve. For orbit 2, R_2=R_1sqrt(T_2/T_1)"

...but I still can't understand what he's talking about. What does he mean that period T is proprtional to r^2? And what does any of this have to do with balancing the centripetal force with the force of gravity?

hint: what is the equation balancing the centripetal acceleration with the gravitational acceleration? :wink:
 

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