Three equations of motion homework

In summary, the conversation discusses using the kinematic equations for uniformly accelerated motion to find the height of a ball thrown vertically upwards. It also mentions using the conservation of energy equation, which involves both kinetic and potential energy, to find the height. The use of gravitational potential energy is also mentioned, which can be used when gravity is involved and a massive object changes position. The conversation ends with the conclusion that the ratio of heights for two different balls thrown at different speeds is 4:1.
  • #1
Viraam
66
2

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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  • #2
You are using the kinematic equations for uniformly accelerated motion. Do you think they would apply?
 
  • #3
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 ##
 
  • #4
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.
 
  • #5
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.
 
  • #6
Use conservation of energy.
 
  • #7
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.
 
  • #8
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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  • #9
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
 

1. What are the three equations of motion?

The three equations of motion are a set of mathematical equations that describe the relationship between an object's position, velocity, acceleration, and time. These equations are:

1. First equation: v = u + at, where v is final velocity, u is initial velocity, a is acceleration, and t is time.

2. Second equation: s = ut + 1/2at^2, where s is displacement, u is initial velocity, a is acceleration, and t is time.

3. Third equation: v^2 = u^2 + 2as, where v is final velocity, u is initial velocity, a is acceleration, and s is displacement.

2. How do I use the equations of motion to solve problems?

To use the equations of motion, you will need to identify the known values for each equation. These values include the object's initial and final velocity, acceleration, displacement, and time. Once you have identified the known values, you can plug them into the appropriate equation to solve for the unknown value.

3. Can I use the equations of motion for any type of motion?

Yes, the equations of motion can be used for any type of motion, including linear, circular, and projectile motion. However, these equations assume that the object is moving with constant acceleration.

4. What is the difference between displacement and distance?

Displacement refers to the change in an object's position from its initial position to its final position. It is a vector quantity, meaning it has both magnitude and direction. Distance, on the other hand, refers to the total length of the path traveled by an object and is a scalar quantity, meaning it only has magnitude.

5. What are the units for the variables in the equations of motion?

The units for the variables in the equations of motion are:

- Velocity (v and u): meters per second (m/s)

- Acceleration (a): meters per second squared (m/s^2)

- Displacement (s): meters (m)

- Time (t): seconds (s)

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