Calculating New Period of a Shrinking Star with Uniform Mass Distribution

In summary: So the final equation will be:Ii * Wi = If * Wf2/5MR^2 * 1rot/36.3 days = (2/5M(0.590R)^2) * WfIn summary, to find the new period of a star with a mass of 1.250×1031 kg and a rotation period of 36.30 days, with a sudden change in diameter to 0.590 times its present size, one must use the conservation of angular momentum equation. By plugging in the given values and using the formula for a solid sphere, the new period can be determined.
  • #1
BuBbLeS01
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0
Period of a Star...Please help!

Homework Statement


The mass of a star is 1.250×1031 kg and it performs one rotation in 36.30 day. Find its new period (in days) if the diameter suddenly shrinks to 0.590 times its present size. Assume a uniform mass distribution before and after.

I don't know where to begin!
 
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  • #2
Think about conservation of angular momentum. What do you know about that?
 
  • #3
Torque(net) * Change in T = Change in L
Ii * Wi = If * Wf
 
  • #4
Ii * Wi = If * Wf

OK, so what do you think you might do next? What is I for a solid sphere?
 
  • #5
2/5MR^2 but how do we get R?
1 rotation/36.3days * pi = W
 
  • #6
You don't need to know the radius. In the question, you are given the final radius in terms of the first, so it will cancel out.

1 rotation/36.3days * pi = W

Be careful. This isn't quite right. If you are going to convert this, remember there are 2*pi radians in one revolution.
 
  • #7
Right that's what I thought, but I don't know how to convert rotations to revolutions...
 
  • #8
1 rotation = 1 revolution. They mean the same thing. There are 2*pi radians per rotation (or revolution).
 
  • #9
You could leave Wi in terms of rotation/day for this particular problem since all of your other units will cancel out. Of course, if you're unsure how to do it, it's good practice to give it a try.
 
  • #10
Ii * Wi = If * Wf
2/5MR^2 * 1rot/36.3 days = If * Wf
I am not sure how we figure out If?
 
  • #11
If will be the same equation where the only thing that changes is R since the star becomes smaller in diameter. You are given information in the question that allows you to determine how much smaller it becomes

Find its new period (in days) if the diameter suddenly shrinks to 0.590 times its present size.
 
  • #12
Ii * Wi = If * Wf
2/5MR^2 * 1rot/36.3 days = (2/5MR^2*0.590) * Wf
 
  • #13
BuBbLeS01 said:
Ii * Wi = If * Wf
2/5MR^2 * 1rot/36.3 days = (2/5MR^2*0.590) * Wf

This needs to be squared as well, since it is part of the radius term.
 

1. What is the period of a star?

The period of a star is the amount of time it takes for the star to complete one full rotation on its axis. It is similar to the concept of a day on Earth, but differs in length depending on the size and type of star.

2. How is the period of a star measured?

The period of a star is measured by observing changes in the star's brightness over time. As a star rotates, different parts of its surface are visible, causing fluctuations in brightness. By tracking these changes, scientists can determine the length of the star's period.

3. What factors affect the period of a star?

The period of a star can be influenced by a variety of factors, including the star's mass, age, and composition. A larger or more massive star will have a shorter period, while a smaller or less massive star will have a longer period. Additionally, stars made up of different elements may have different periods due to variations in their internal structures.

4. Why is the period of a star important?

Studying the period of a star can provide valuable insights into its physical properties and evolution. It can also help scientists understand how stars interact with their surrounding environments and how they contribute to the overall structure and dynamics of the universe.

5. Can the period of a star change over time?

Yes, the period of a star can change over time due to a variety of factors, such as interactions with other stars or objects in its vicinity, or changes in its internal structure. However, these changes are usually gradual and can only be observed over long periods of time.

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