How Do You Calculate Forces in Centripetal Motion Problems?

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SUMMARY

This discussion focuses on calculating forces in centripetal motion problems, specifically addressing homework questions involving banked curves, orbital mechanics, and gravitational forces. Key equations include the centripetal force formula, which relates velocity, radius, and mass, and the gravitational force equation for celestial bodies. The discussion highlights the importance of understanding static friction in banked curves and the relationship between orbital speed and mass for stars and black holes. Participants emphasize the need for a solid grasp of these concepts to solve the posed problems effectively.

PREREQUISITES
  • Centripetal force calculations
  • Understanding of gravitational force equations
  • Knowledge of static friction in banked curves
  • Familiarity with orbital mechanics and Kepler's laws
NEXT STEPS
  • Study the derivation of centripetal force equations
  • Learn about gravitational force calculations for celestial bodies
  • Explore the effects of static friction on banked curves
  • Investigate the relationship between orbital speed and mass in astrophysics
USEFUL FOR

Students in physics, educators teaching mechanics, and anyone interested in understanding the principles of centripetal motion and gravitational forces in both terrestrial and astronomical contexts.

Stephanie
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I have a few homework problems do tomorrow and I have tried and can't figure out these few problems. Thanks for the help. Oh and I don't just want the answers. I have those...I need help forming the equations. Thanks.

73. A curve of radius 60m is banked for a design speed of 100km/hr. If the coefficient of static friction is .30 (wet pavement), at what range of speeds can a car safely make the curve?

75. Two equal-mass stars maintain a constant distance apart of 8.0 x 10^10m and rotate about a point mid-way between them at a rate of one revolution every 12.6yrs. What must be the mass of each star?

76. A train traveling at a constant speed rounds a curve of radius 275m. A chandelier suspended from the ceiling swings out to an angle of 17.5degrees throughout the turn. What is the speed of the train?

78. Astronomers using the Hubble Space Telecope have recently deduced the presence of an extremely massive core in the distant galazy M87, so dense that it could well be a black hole. They did this by measuring the speed of gas clouds orbiting the core to be 780km/s at a distance of 60Lightyears (5.7x10^17m) from the core. Deduce the mass of the core and compare it to the mass of our sun.

**I think that 78 is just Velocity^2 divided by radius, is that right?
 
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-73- looks familiar. I think it came up a few days ago, but my quick search didn't find it. Here's a related thread with a long discussion of friction and banked tracks, though:

https://www.physicsforums.com/showthread.php?t=135880

-78- no, I don't think you have the correct approach (and I don't understand your approach). What do you use to calculate the mass of the Earth or another large body in space, given the orbital distance and speed? Do you need the mass of the orbiting object? (Hint -- remember that you can put satellites in geostationary orbit, independent of their mass.)
 
Stephanie said:
...75. Two equal-mass stars maintain a constant distance apart of 8.0 x 10^10m and rotate about a point mid-way between them at a rate of one revolution every 12.6yrs. What must be the mass of each star?

Which is the force that crosses your mind when rotation is mentioned? Further on, what force crosses your mind when two celestial objects are mentioned? What is the relation between these two forces?
 

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