Three equations of motion homework

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Homework Help Overview

The discussion revolves around the application of the three equations of motion in the context of gravitational motion, specifically regarding the maximum height reached by an object under uniform acceleration due to gravity.

Discussion Character

  • Exploratory, Assumption checking

Approaches and Questions Raised

  • Participants explore the applicability of kinematic equations for uniformly accelerated motion, questioning whether they are suitable given the context of gravitational acceleration.
  • Some participants express uncertainty about how to find heights and seek clarification on the relevant formulas, indicating a need for conceptual understanding of gravitational potential energy.
  • There are discussions about the definitions and equations related to gravitational potential energy, with participants questioning when it is appropriate to use this concept.

Discussion Status

The conversation is ongoing, with participants sharing their understanding and seeking clarification on the use of gravitational potential energy. Some guidance has been offered regarding the equations involved, but there is no explicit consensus on the application of the three equations of motion in this context.

Contextual Notes

Participants note that they have not fully learned about gravitational potential energy and are working within the constraints of their current curriculum, which includes specific equations related to gravitational force and acceleration.

Viraam
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Homework Statement


ck_55fc3aad67048.png


Homework Equations


## 2as = v^2-u^2 ##
## v = 0 ... \text{at maximum height}##
## \therefore s = \frac{-(u)^2}{2a} \\ a = -g \\ \therefore s = \frac{-(u)^2}{-2g} = \frac{(u)^2}{2g} ##
Please explain using only the Three equations of motion and not anything related to Energy or other formulae.

The Attempt at a Solution


Is my answer correct:-
ck_55fc3ab91ae5e.png
 
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You are using the kinematic equations for uniformly accelerated motion. Do you think they would apply?
 
Doc Al said:
You are using the kinematic equations for uniformly accelerated motion. Do you think they would apply?
Yeah. Because they are uniformly accelerated to ## g ##
 
Viraam said:
Yeah. Because they are uniformly accelerated to ## g ##
The acceleration is ## g ## when the balls are close to the Earth's surface. But those speeds are pretty high.
 
Doc Al said:
The acceleration is ## g ## when the balls are close to the Earth's surface. But those speeds are pretty high.
Ohh then please tell me how to find the Heights.
 
Use conservation of energy.
 
Doc Al said:
Use conservation of energy.
We haven't learned that. Can you please tell me the formula.
Some other sites states the following:-
##KE + PE \text{ at the surface} = PE \text{ at the maximum height}##
Can you please explain in simpler words because I am very new to this.
 
Viraam said:
We haven't learned that. Can you please tell me the formula.
Some other sites states the following:-
##KE + PE \text{ at the surface} = PE \text{ at the maximum height}##
Can you please explain in simpler words because I am very new to this.
That's exactly the equation you need. Of course you need to learn how to express the gravitational PE.

If you haven't studied this yet, where did you get the problem?
 
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We haven't learned it completely yet. But this question was in our chapter called Gravitation.
 
  • #10
Viraam said:
We haven't learned it completely yet. But this question was in our chapter called Gravitation.
Good. So it should cover how you calculate the gravitational PE at some distance from a planet.
 
  • #11
No we learned only these equations:-
##F = \frac{GMm}{R^2}\\ g = \frac{GM}{R^2}##
Do you mean this:-
## PE = mgh##
## PE = \frac{GMmh}{R^2}##
 
  • #15
Viraam said:
So the answer is 4:1
How did you determine that?
 
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  • #16
Doc Al said:
How did you determine that?
Using
## KE + PE \text{ at surface} = PE \text{ at maximum height} ##
## \frac{1}{2} m *(2\sqrt{\frac{gR}{3}})^2 - \frac{GMm}{R}= \frac{-GMm}{R+h}\\
h = 2 R\\ \text{For the other ball:-} \\ h' = \frac{R}{2}\\ \frac{h}{h'} = \fbox{4:1}\\ ##
 
  • #17
Viraam said:
Using
## KE + PE \text{ at surface} = PE \text{ at maximum height} ##
## \frac{1}{2} m *(2\sqrt{\frac{gR}{3}})^2 - \frac{GMm}{R}= \frac{-GMm}{R+h}\\
h = 2 R\\ \text{For the other ball:-} \\ h' = \frac{R}{2}\\ \frac{h}{h'} = \fbox{4:1}\\ ##
Looks right to me. Well done.
 
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  • #18
Viraam said:
Using
## KE + PE \text{ at surface} = PE \text{ at maximum height} ##
## \frac{1}{2} m *(2\sqrt{\frac{gR}{3}})^2 - \frac{GMm}{R}= \frac{-GMm}{R+h}\\
h = 2 R\\ \text{For the other ball:-} \\ h' = \frac{R}{2}\\ \frac{h}{h'} = \fbox{4:1}\\ ##
Good work! (Just wanted to check. :smile:)
 
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  • #19
Doc Al said:
Good work! (Just wanted to check. :smile:)
Have a doubt. How exactly do we know when to use Gravitational Potential Energy. Please explain in the simplest words. Thanking you in advance.
 
  • #20
Viraam said:
Have a doubt. How exactly do we know when to use Gravitational Potential Energy. Please explain in the simplest words.
That's difficult to answer. Just stating the obvious: When gravity is involved and a massive object changes position, you may be able to make use of gravitational PE. But it depends on the problem and what you need to find.
 
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  • #21
Doc Al said:
That's difficult to answer. Just stating the obvious: When gravity is involved and a massive object changes position, you may be able to make use of gravitational PE. But it depends on the problem and what you need to find.
Ohh ok Thank you so much
 

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