Angular Momentum Conservation Problem

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Homework Help Overview

The discussion revolves around a problem related to the conservation of angular momentum in the context of stellar evolution, specifically the transition of a star into a white dwarf state. The original poster presents a scenario involving a star with specific mass and rotation characteristics before and after its transformation.

Discussion Character

  • Exploratory, Assumption checking, Mathematical reasoning

Approaches and Questions Raised

  • Participants discuss the application of angular momentum conservation principles, particularly focusing on the relationship between the initial and final states of the star's mass, radius, and rotation period. There are inquiries about potential errors in calculations and formulas used, as well as the accuracy of results obtained from different calculators.

Discussion Status

The conversation reflects a mix of attempts to verify calculations and explore discrepancies in results. Some participants have reached similar conclusions, while others express uncertainty about the correctness of their answers. There is no clear consensus on the validity of the results, and suggestions to consult external resources, such as a teacher, have been made.

Contextual Notes

Participants note variations in mass values and their impact on calculations, highlighting the importance of precision in numerical inputs. There is also mention of the constraints imposed by the homework platform, which may influence the perceived correctness of answers.

akan
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Homework Statement


When a star like our Sun no longer has any hydrogen or helium "fuel" for thermonuclear reactions in its core, it can collapse and become a white dwarf star. Often the star will "blow off" its outer layers and lose some mass before it collapses into the rapidly spinning, dense white dwarf. Suppose a star with mass 1.0 Msun, with a radius of 6.96×10^8 m and rotating once every 25 days, becomes a white dwarf with a mass of 0.62 Msun and a rotation period of 131 s.


Homework Equations


Msun = 1.99 × 1030 kilograms
M1 = 1.0 Msun
R1 = 6.96 * 108
T1 = 25 days = 2 160 000 seconds

M2 = 0.62 Msun
R2 = ?
T2 = 131 seconds

T = 2 pi r / v
= 2 pi r / w r
= 2 pi / w
.:. w = 2 pi / T

I = (2/5)MR2

The Attempt at a Solution


I1 x w1 = I2 x w2
(2/5)(M1 x R12)(2 pi / T1) = (2/5)(M2 x R22)(2 pi / T2)
(M1 x R12)(1 / T1) = (M2 x R22)(1 / T2)
(M1 / M2)(T2 / T1)(R12) = R22
sqrt((M1 / M2)(T2 / T1)(R12)) = R22
R2 = sqrt((1.99*1030)/[(0.62)(1.99*1030)](131/2160000)(6.96*108)2
= 6.88*106 m

Checking the result by plugging into equations shows that I am roughly correct. But Mastering Psychics says I am wrong. Where is the mistake?
 
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I get a different answer using your last equation. Perhaps you typed it into your calculator incorrectly?
 
Well, I tried typing it a few more times and I am still getting the same answer. I also tried to use the masteringphysics integrated calculator, which is more graphical, but got the same answer. What answer do you get? And are there any errors in any of my formulas?
 
Hmmm, I think I might have typed it into my calculator wrong since I now get the same answer as you. :redface: As far as I can tell, your solution is correct. Perhaps check with your teacher to see if the answer given is wrong?
 
I have the similar problem as you are except my mass is .6 M_{sun} now when pluggin mine in I get the following equation:

R_{2} = \sqrt{\frac{1.99x10^{30}}{(.60 * 1.99x10^{30})} * \frac{131}{2160000} * 6.96x10^{8}} = 70351.8 = 70000 if you do 2 sig figs, but according to mastering physics is wrong so any help on where its going wrong would suffice.
 

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