Centripetal acceleration where to start

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SUMMARY

The discussion centers on calculating the centripetal acceleration of a car traveling at a constant speed around a circular track with a radius of 2.63 km, completing one lap in 353 seconds. The key formula for centripetal acceleration, A = V²/r, is highlighted, where V is the speed of the car and r is the radius of the track. To find the speed, the circumference of the track is calculated using the formula C = 2πR, and then divided by the time taken to complete the lap. By substituting the calculated speed into the centripetal acceleration formula, the solution can be derived.

PREREQUISITES
  • Understanding of circular motion and centripetal acceleration
  • Familiarity with the formulas for circumference and centripetal acceleration
  • Basic algebra for manipulating equations
  • Knowledge of units of measurement (e.g., converting km to m)
NEXT STEPS
  • Calculate the circumference of a circle using C = 2πR
  • Learn how to derive speed from distance and time
  • Practice problems involving centripetal acceleration using different radii and times
  • Explore the relationship between speed and centripetal force in circular motion
USEFUL FOR

Students studying physics, particularly those focusing on mechanics and circular motion, as well as educators looking for practical examples of centripetal acceleration calculations.

Caitiemarie89
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Homework Statement



A car travels at a constant speed around a circular track whose radius is 2.63 km. The car goes once around the track in 353 s. What is the magnitude of the centripetal acceleration of the car?

Homework Equations



A=V^2/r C=1/2(pi)R^2


The Attempt at a Solution


I have no clue where to start on this question
 
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Don't think this should be in the 'advanced physics' section!

The speed of the car will be the circumference of the track, divided by the time it takes for the car to go around once. You've written down the formula for centripetal acceleration a=v^2/r so plug in the values and out pops the answer!
 

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