Centripetal force and orbital motion....

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Discussion Overview

The discussion revolves around the relationship between centripetal force and gravitational force in various types of motion, particularly focusing on projectile motion, parabolic paths, and orbital dynamics. Participants explore whether centripetal force can be equated to gravitational force in different scenarios, including hypothetical situations involving motion through Earth.

Discussion Character

  • Exploratory
  • Technical explanation
  • Conceptual clarification
  • Debate/contested

Main Points Raised

  • Some participants propose that centripetal forces are present in any curved path, not limited to circular motion, and that in parabolic motion, the centripetal force is related to the component of gravitational force perpendicular to the path.
  • Questions arise regarding the definition of radius in the context of a parabola, as the centripetal force formula includes a radius term.
  • Participants discuss the components of acceleration in curved motion, noting that tangential and normal components exist for any curve, including parabolic and circular paths.
  • One participant queries whether the centripetal force is less than, equal to, or greater than gravitational force in different types of projectile motion (parabolic, circular, and elliptical).
  • Responses indicate that in projectile motion under gravity, the normal (centripetal) component is less than gravitational force, while in circular motion, it may equal gravitational force, and in elliptical motion, it is suggested that the normal component is smaller than gravitational force.
  • Some participants express uncertainty about the role of gravity in circular and elliptical motion, suggesting that gravity alone may not account for the motion in these cases.

Areas of Agreement / Disagreement

Participants do not reach a consensus on the relationship between centripetal force and gravitational force across different types of motion, with multiple competing views and uncertainties remaining in the discussion.

Contextual Notes

Participants highlight the complexity of defining the radius of curvature for non-circular paths and the interplay between tangential and normal components of acceleration in various motion scenarios.

ViolentCorpse
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Hi,

The force of gravity is the centripetal force when an object is in motion. But in projectile motion, where the speed is not enough to keep it in orbit, could the force of gravity be equated to centripetal force?

I'm trying to understand if all types of curved motion can be explained by centripetal force, or put differently, instances where the concept of centripetal force applies. For example, if a projectile is allowed to fall right through Earth matter (instead of colliding with the ground (in our imagination, of course)), would it be able to orbit it in some kind of weird curve? Would the centripetal force apply here? If it can, then it must have to be different than the force of gravity, which is strange because centripetal force is always just a manifestation of some other force and the only force involved in projectile/satellite motion is gravity..

I hope you guys are getting my point..
 
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Centripetal forces exist on any curved path, not just a circular path. For parabolic motion under gravity only, the centripetal force at any point is the component of the gravity force perpendicular to the tangent of the path at that point
 
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PhanthomJay said:
For parabolic motion under gravity only, the centripetal force at any point is the component of the gravity force perpendicular to the tangent of the path at that point
Interesting!

There is, however, a radius term in the formula of centripetal force. What could be the radius of a parabola?
 
ViolentCorpse said:
Interesting!

There is, however, a radius term in the formula of centripetal force. What could be the radius of a parabola?
In motion along any plane curve, there are two components of acceleration, tangential and normal. The tangential component is equal to dv/dt, where v is the speed. The normal component is equal to v^2/r where v is the speed and r is the radius of curvature. This is correct for any curve, parabolic, circular, or arbitrary.
 
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Chandra Prayaga said:
In motion along any plane curve, there are two components of acceleration, tangential and normal. The tangential component is equal to dv/dt, where v is the speed. The normal component is equal to v^2/r where v is the speed and r is the radius of curvature. This is correct for any curve, parabolic, circular, or arbitrary.
Makes perfect sense! Thanks so much! :)

There's just one more thing I must ask: Is the centripetal force less than the force due to gravity when the curve of a projectile is parabolic, equal to gravity when it is circular and greater than gravity when it is elliptic?
 
ViolentCorpse said:
Makes perfect sense! Thanks so much! :)

There's just one more thing I must ask: Is the centripetal force less than the force due to gravity when the curve of a projectile is parabolic, equal to gravity when it is circular and greater than gravity when it is elliptic?
1. Projectile motion with only gravity: The two components, tangential and normal, must together add as vectors to give the downward acceleration due to gravity, so the normal (centripetal) component will be numerically less than g.
2. Circular or elliptical motion: If we are still talking about motion on the earth, I don't see gravity alone being responsible for either circular or elliptical motion, so the comparison cannot be made.
3. Planetary motion with a single center of force: If the motion is circular, then it is also with constant speed, so there is no tangential component of acceleration, and the normal component is exactly equal to gravity. If the motion is elliptical, the gravitational force contributes to the normal component and the tangential component, so the normal component will be numerically smaller than the gravitational force/mass.
 
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Thank you so much! :)
 

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