- #1
Doc Al said:You need to find the tension as a function of angle. (Forget the tension at the top.)
You have the correct equation. Hint: Express v^2 as a function of angle.
Doc Al said:The equation I had in mind was: mv^2/r = T + mg cos(theta).
Another hint: What's conserved as the ball continues on its path?
The velocity is definitely not constant. Reread my hint in post #4.asi123 said:I got stuck because I don't know the velocity at this point, I mean, the velocity is not constant, right?
Doc Al said:The velocity is definitely not constant. Reread my hint in post #4.
Given the velocity at the top, you should be able to find the velocity at any point as a function of angle.
Getting warmer!asi123 said:Oh, maybe u mean to use energy calculation?
Doc Al said:Getting warmer!
Looks good to me.asi123 said:Ok, I haven't really learned Conservation of energy so I'm not really familiar with it...
I wrote this equation about the energy, is it correct?
Excellent question! Ask yourself: Does the tension force do any work on the ball?And another thing, What about T? it's not a Conservative force, right? Do I just ignore it in the the energy equation?
Doc Al said:Looks good to me.
Excellent question! Ask yourself: Does the tension force do any work on the ball?
Circular movement is the motion of an object or particle along a circular path. It is important because it can be found in many natural phenomena, such as the orbit of planets around the sun, the rotation of the Earth, and the motion of electrons around an atom. It is also used in various machines and technologies, such as gears, pulleys, and centrifuges.
Uniform circular motion is when an object moves along a circular path at a constant speed, while non-uniform circular motion is when the speed of the object changes at different points along the path. In uniform circular motion, the object experiences a constant centripetal acceleration, while in non-uniform circular motion, the acceleration varies in direction and magnitude.
Centripetal force is the force that keeps an object in circular motion. It is always directed towards the center of the circular path and is equal to the product of the object's mass, its speed squared, and the radius of the circular path. Without a centripetal force, an object would continue in a straight line instead of following a circular path.
Some real-life examples of circular motion include the motion of a Ferris wheel, the orbit of satellites around the Earth, the spin of a top, and the rotation of a ceiling fan. Other examples include the swinging of a pendulum, the motion of a car around a curve, and the motion of a planet around its star.
To solve problems involving circular motion, you can use equations such as centripetal force = mass x speed² / radius, centripetal acceleration = speed² / radius, and velocity = 2πr / T (where r is the radius and T is the period). It is important to clearly define the variables and units in the problem and choose the appropriate equation to solve for the desired quantity.