Calculating the Moment of Inertia of the Sun for Determining Rotational Energy

Click For Summary
SUMMARY

The discussion focuses on calculating the moment of inertia of the Sun to determine its rotational energy using the formula Erot=1/2*I*ω². The user initially applies the moment of inertia formula for a uniform sphere, I=2/5*m*r², yielding a value of 3.848671797*10^47 km*m². However, due to the Sun's non-uniform density, an empirical value is recommended, specifically I/MR² = 0.059, which contrasts sharply with the uniform density sphere's value of 0.4. This empirical approach is essential for accurate calculations in astrophysics.

PREREQUISITES
  • Understanding of rotational energy equations in physics
  • Familiarity with moment of inertia concepts
  • Basic knowledge of astrophysics and the Sun's structure
  • Ability to interpret empirical data from scientific sources
NEXT STEPS
  • Research the empirical values for moment of inertia in celestial bodies
  • Study the differences between uniform and non-uniform density models
  • Learn about the Sun's internal structure and density distribution
  • Explore advanced astrophysics concepts related to rotational dynamics
USEFUL FOR

Astrophysicists, physics students, and anyone interested in celestial mechanics and the dynamics of the Sun.

AndersLau
Messages
4
Reaction score
0
I want to find the rotational energy of the sun.
Erot=1/2*I*ω2

m=1.9891*10^30 kg
r=6.955*10^5 km


When I am using the formula for a sphere's moment of inertia: I=2/5*m*r2
I'm getting 3.848671797*1047 km*m2

Can i find the moment of inertia in another way? the moment of inertia needs to be in *1046 , to get the rotational energy right.

Thank you.
 
Physics news on Phys.org
A uniform density sphere is a fairly bad model even for the earth, which is more or less solid. For a gas it is an incredibly lousy model. The sun's core contains about half of the total mass of the sun but only 1.5% of its total volume.

Unless you want to get into astrophysics, you are going to need an empirical value. From http://nssdc.gsfc.nasa.gov/planetary/factsheet/sunfact.html, I/MR2 for the sun is 0.059. Compare that for a uniform density sphere, where I/MR2=2/5 or 0.4.
 
Thank you very much for the answer, that sorts it out. Much appreciated.
I'm waiting with the astrophysics :)
 

Similar threads

Replies
2
Views
2K
  • · Replies 40 ·
2
Replies
40
Views
6K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 28 ·
Replies
28
Views
2K
Replies
11
Views
3K
  • · Replies 8 ·
Replies
8
Views
1K
Replies
25
Views
2K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 3 ·
Replies
3
Views
1K
  • · Replies 3 ·
Replies
3
Views
2K