Solving Circular Motion Problems: Finding Centripetal Acceleration and Velocity

In summary: It may hold true for objects at the Earth's surface, but the problem is talking about orbiting at a distance of 400km from the surface. Therefore, the gravitational acceleration will be different.
  • #1
jrd007
159
0
I think I did the problem(s) right but my answers doesn't match up with the correct answer.

1) Suppose a space shuttle is in orbit 400km from the Earth's surface, and circles the Earth once every 90 minutes. Find the centripital acceleration of the space shuttle's orbit. Express your answer in terms of g, the gravitational acc. or the Earth's surface.

Okay, so my approach:
First change 400km into m = 40,000m & 90min = 5400s

So since a=v^2/r, I will find velocity first. So I used Vel=2(pie, 3.14)(r)/t
(2 x 3.14 x 40,000m)/5400s = 465.4 m/s

Then I took a=v^2/r. So ... a=465.4^2/40,000m and got .541 m/s^2

Then convert into g's, .541/9.8 = .06 g
But the correct answer is 0.9 g's What am I doing wrong!? :(


2) What is the max speed w/ which a 1050-kg car can round a turn with a radius of 77m on a flat road if the coefficent of static friction b/t tires and road is 0.80?

What I tried to do was find my acceleration so I could get my velocity but I have no idea how to do that? Since the velocity is not given... Can anyone help me? Correct answer: 25 m/s
 
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  • #2
jrd007 said:
I think I did the problem(s) right but my answers doesn't match up with the correct answer.

1) Suppose a space shuttle is in orbit 400km from the Earth's surface, and circles the Earth once every 90 minutes. Find the centripital acceleration of the space shuttle's orbit. Express your answer in terms of g, the gravitational acc. or the Earth's surface.

Okay, so my approach:
First change 400km into m = 40,000m & 90min = 5400s

So since a=v^2/r, I will find velocity first. So I used Vel=2(pie, 3.14)(r)/t
(2 x 3.14 x 40,000m)/5400s = 465.4 m/s

Then I took a=v^2/r. So ... a=465.4^2/40,000m and got .541 m/s^2

Then convert into g's, .541/9.8 = .06 g
But the correct answer is 0.9 g's What am I doing wrong!? :(


2) What is the max speed w/ which a 1050-kg car can round a turn with a radius of 77m on a flat road if the coefficent of static friction b/t tires and road is 0.80?

What I tried to do was find my acceleration so I could get my velocity but I have no idea how to do that? Since the velocity is not given... Can anyone help me? Correct answer: 25 m/s
The shuttle is 400km from the surface of the earth. You need to find the distance from the center of the earth.

Alex
 
  • #3
jrd007 said:
Okay, so my approach:
First change 400km into m = 40,000m & 90min = 5400s

So since a=v^2/r, I will find velocity first. So I used Vel=2(pie, 3.14)(r)/t
(2 x 3.14 x 40,000m)/5400s = 465.4 m/s


You forgot to add in the Earth's radius of about 6500km ! That makes a big difference. Try it again.

jrd007 said:
2) What is the max speed w/ which a 1050-kg car can round a turn with a radius of 77m on a flat road if the coefficent of static friction b/t tires and road is 0.80?

What I tried to do was find my acceleration so I could get my velocity but I have no idea how to do that? Since the velocity is not given... Can anyone help me? Correct answer: 25 m/s

First of all, find the maximum frictional force that can act on the 1050kg car given the coefficient of 0.8. Now with that find the corresponding acceleration possible. From there you know the acceleration is radial, so you can apply it to circular motion :)
 
  • #4
mezarashi said:
You forgot to add in the Earth's radius of about 6500km ! That makes a big difference. Try it again.



First of all, find the maximum frictional force that can act on the 1050kg car given the coefficient of 0.8. Now with that find the corresponding acceleration possible. From there you know the acceleration is radial, so you can apply it to circular motion :)

That worked... but how was I suppose to know the radius of the earth?
 
  • #5
Haha, I'd guess it would more or less become common knowledge sooner or later. Physics major? Look at the back of your textbook's cover, such figures are usually available or else, try googling: Earth's diameter

In anycase, it should have been clear that that information was missing.
 
  • #6
mezarashi said:
Haha, I'd guess it would more or less become common knowledge sooner or later. Physics major? Look at the back of your textbook's cover, such figures are usually available or else, try googling: Earth's diameter

In anycase, it should have been clear that that information was missing.

Umm... Sorry, this is my first semester of Physics. I am just trying to get through.
 
  • #7
Yep I got an a=0.95 g's. Now I'll try the other problem.
 
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  • #8
Check your math: 6900km = 6,900,000m (just for the record, the better estimate for the Earth's radius is 6378km for an equatorial orbit)

The answer of 0.9g is very reasonable. This means that moving 400km off the surface of the Earth, the gravitational force will feel will be 0.9 times what we feel here on the surface.
 
  • #9
Okay, now for the second problem. I have finished the first part but am still stuck... Okay...

I get the max tension/force by first getting the Normal force like so...

(1050kg) x (9.8 m/s^2) = 10290 N

Then I take my static coeffiecent of .80 and times it by 10290N
(.80) x (10290N) = 8232 N as my max frictional force

But how can I get the velocity from this? The equations don't seem to work...
 
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  • #10
Now how do I get the velocity? :S
 
  • #11
The equations don't work? Think carefully. What is this frictional force working against. Or rather, what does this frictional force represent? Why does it exist? We're talking about circular motion and centripetal acceleration here remember.
 
  • #12
So, I cannot use v= square root of (F/m x r) ?
 
  • #13
You might need to use parentheses in your calculator ... .

by the way, the first problem can also be answered using
gravity field strength g proportional to 1/r^2 :
a/"g_surface" = R^2 / (R+h)^2
 
  • #14
lightgrav said:
You might need to use parentheses in your calculator ... .

by the way, the first problem can also be answered using
gravity field strength g proportional to 1/r^2 :
a/"g_surface" = R^2 / (R+h)^2
So the equation will work for problem 2?
 
  • #15
Look, the only horizontal Force, the only one with a center-pointing component, is the friction Force. The sum of the central Force components provides m with a_central , which is v^2/r . Just like ANY OTHER known component of acceleration is caused by that Force component Sum.

The diagrams are ALWAYS the key to Physics problems ...
Your diagram should've shown the satellite with a circular path that had a radius of R+h. That's how you know to look up R inside the book cover, and suggests that you could solve the problem by looking at gravitational Force.

This Free-Body Diagram is simple enough that you should have a lot of confidence in your result ... a = (.8)(9.8 m/s^2) = v^2/r
 
  • #16
I still do not understand, but thanks for trying.
 
  • #17
If you isolate "v" in the equation: a = v^2/r ,
yes, you get v^2 = ar , so ... v = sqrt(ar).
F/m ... which you had long back ... IS "a" .
 
  • #18
So it would be sqrt (F/m) x r ) (8232 N/1050kg) x 77 = 24.5 = 25.0 ! It worked!
 
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FAQ: Solving Circular Motion Problems: Finding Centripetal Acceleration and Velocity

1. What is circular motion and why is it important to understand?

Circular motion is the movement of an object along a circular path. It is important to understand because many objects in our daily lives, such as planets orbiting the sun or cars turning on a curved road, undergo circular motion. Understanding circular motion allows us to analyze and predict the behavior of these objects and make informed decisions.

2. What is centripetal acceleration and how is it different from regular acceleration?

Centripetal acceleration is the acceleration towards the center of a circular path. It is different from regular acceleration because it only changes the direction of an object's velocity, not its speed. In circular motion, the object's speed remains constant, but the direction of its velocity changes constantly.

3. How do you calculate the centripetal acceleration of an object?

The formula for centripetal acceleration is a = v^2/r, where a is the acceleration, v is the velocity of the object, and r is the radius of the circular path. This means that the centripetal acceleration is directly proportional to the square of the object's velocity and inversely proportional to the radius of the circular path.

4. How do you find the velocity of an object in circular motion?

The formula for velocity in circular motion is v = 2πr/T, where v is the velocity, r is the radius of the circular path, and T is the time it takes for the object to complete one full revolution. This means that the velocity is directly proportional to the radius and inversely proportional to the time taken to complete one revolution.

5. What are some real-life examples of circular motion problems?

Some real-life examples of circular motion problems include the motion of a Ferris wheel, the orbit of a satellite around the Earth, and the motion of a spinning top. These objects all move along a circular path and can be analyzed using the principles of circular motion to determine their centripetal acceleration and velocity.

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