Direction of normal acceleration problems

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SUMMARY

The discussion centers on the concept of normal acceleration in circular motion, specifically addressing the equations governing forces acting on an object in motion. The key equations discussed include the normal force component Nc sin θ = mv² / r and the relationship mg = Fc + N, where Fc represents the centripetal force. Participants clarify that Fc is not an independent force but a resultant force necessary for circular motion, emphasizing the importance of understanding the net forces acting on an object to maintain uniform circular motion.

PREREQUISITES
  • Understanding of Newton's laws of motion
  • Familiarity with circular motion dynamics
  • Knowledge of free body diagrams
  • Basic concepts of centripetal force and acceleration
NEXT STEPS
  • Study the derivation of centripetal acceleration formulas
  • Learn about the role of normal force in inclined circular motion
  • Explore the concept of resultant forces in physics
  • Review examples of free body diagrams in circular motion scenarios
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Students studying physics, particularly those focusing on mechanics, as well as educators seeking to clarify concepts of forces in circular motion.

yugeci
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Homework Statement



0e83fbb3c833a476678e61442361a40d.png


Homework Equations



An = mv^2 / r

The Attempt at a Solution



I get the 2D free body diagram, and how the vertical components are resolved, but how is Nc sin θ = mv^2 / r when they both are in the same direction?

Also another related problem is this diagram here:

364dd07c469b6d3c525859cb6b79e8ae.png


The equation for the mass at B is,

mg = Fc + N

How is this so when both Mg and Fc are directed downwards (Fc being the centripetal force mv^2 / ρ). Shouldn't it be mg + Fc = N?

I guess I don't understand the direction of Fc due to the normal acceleration. in either of these problems.
 
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"when they both are in the same direction?" is not all that clear to me. Who is in which direction, and who else ?

In your second problem, a conceptual dwelling becomes a bit clearer.
Basically, there is no Fc. For an object to execute a circular motion, some force has to play that role.

In the first problem, the horizontal component of the normal force plays that role. Hence also the equality Nc sin θ = mv^2 / r.

In the second problem, the vertical component of the gravitational force plays that role. Not all of it, so there remains some normal force. (**)

A "much better" (ahem) way to write this would be mg - N = the force to cause a circular motion.

Since we generally like short notation, we often use Fc for "the force to cause a circular motion", so now that name is back again. But remember it is shorthand for "the force to cause a circular motion" (or the force that changes the direction of the velocity vector...)

(**) Well, if v is big enough, all of mg is needed to keep the object on the circular trajectory. Increasing v beyond that, the car will loose contact with the hill, since there are no other contribuant forces that might keep it on there.

[edit] Ah, I see it's not a car but an unspecified "mass". Story doesn't change.
 
yugeci said:
I get the 2D free body diagram, and how the vertical components are resolved, but how is Nc sin θ = mv^2 / r when they both are in the same direction?
Both what? I only see one force here: Nc. It has a component in the n direction. The rest is Newton's 2nd law.


Also another related problem is this diagram here:

364dd07c469b6d3c525859cb6b79e8ae.png


The equation for the mass at B is,

mg = Fc + N

How is this so when both Mg and Fc are directed downwards (Fc being the centripetal force mv^2 / ρ). Shouldn't it be mg + Fc = N?

The way to understand it is to think of the net force at B: ∑F = mg - N. (mg is downward, N is upward) That net force is the Fc, so Fc = mg - N. Note that Fc acts downward.
 
Because it's so important, I throw in another reply:

In the top problem, there are only two forces working on the car: gravity and normal force. The (vector) sum of those is not zero due to the incline.

We have learned F = ma (but actually it is ##\vec F = m \vec a##). Where F is the net sum of all forces.

Furthermore, we have learned that for uniform circular motion an acceleration towards the center is needed with a magnitude mv2/r

So if we want the object (car, block, ..) to execute a uniform circular motion, we must ensure that the net sum of forces is pointing the right way (exactly towards the center) and has the magnitude mv2/r.

If you look upon Fc as something that is a resultant instead of one of the forces present, you almost can't go wrong.
 
I see. I thought of Fc as another independent force. It makes sense now. Thanks for all of the replies.
 
BvU said:
If you look upon Fc as something that is a resultant instead of one of the forces present, you almost can't go wrong.
This is an important point. Fc is a resultant (or net) force, not a separate force of its own. Fc should never appear in a free body diagram.
 
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