Is angular momentum conserved in a Supernova?

In summary: So even for a super nova, the fragments would be around 100 times the mass of the sun and only have an angular momentum around 1/10,000th the sun's.
  • #1
FallenApple
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I can see how it would be conserved for the situation of a star turning into a white dwarf since the object is just contracting. Just like the classic ice skater example.

But what about a super nova? Say a star with spin up goes supernova and that the remaining black hole also has spin up but is rotating much faster.

Does that mean that the remaining fragments will have a total angular momentum vector that is pointing down? Let's assume that not only is the spin rate faster, but the angular momentum vector itself is larger upwards for the black hole after supernova compared to the upwards vector before as a star. Mathematically, we need an angular momentum vector that is pointing down so that the vector sum is the same as the angular momentum pre-explosion.

Also, conservation makes sense, since there is no external torque form anywhere else in the universe during the implosion/explosion.

But what would this mean? Does it mean that on average, the flying fragments would have spin down?
 
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  • #2
FallenApple said:
I can see how it would be conserved for the situation of a star turning into a white dwarf since the object is just contracting. Just like the classic ice skater example.

But what about a super nova? Say a star with spin up goes supernova and that the remaining black hole also has spin up but is rotating much faster.

Does that mean that the remaining fragments will have a total angular momentum vector that is pointing down? Let's assume that not only is the spin rate faster, but the angular momentum vector itself is larger upwards for the black hole after supernova compared to the upwards vector before as a star. Mathematically, we need an angular momentum vector that is pointing down so that the vector sum is the same as the angular momentum pre-explosion.

Also, conservation makes sense, since there is no external torque form anywhere else in the universe during the implosion/explosion.

But what would this mean? Does it mean that on average, the flying fragments would have spin down?

You have to consider that the contraction effect exists on the black hole too. The angular velocity of the black hole might be increased just due to its rotational inertia decreasing (the ice skater effect). Of course the total sum of all momenta still has to be conserved.
 
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  • #3
Yeah, you forgot that black holes are puny compared to stars. Stars that go boom are at least 8 times the mass of our sun and the sun is a million km across, a neutron star is maybe a dozen.
 
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1. What is angular momentum?

Angular momentum is a measurement of an object's rotational momentum, which is a combination of its mass, velocity, and distance from a central axis of rotation.

2. How is angular momentum conserved in a Supernova?

In a Supernova, the core of a massive star collapses and explodes, releasing an enormous amount of energy. This energy is distributed in all directions, including rotationally. As a result, the angular momentum of the star is conserved, but it may be distributed differently among the debris and surrounding space.

3. What factors affect the conservation of angular momentum in a Supernova?

The conservation of angular momentum in a Supernova is affected by the mass and size of the star, as well as the amount of energy released during the explosion. Other factors, such as the star's magnetic field and the presence of a companion star, may also play a role.

4. How does the conservation of angular momentum in a Supernova impact the formation of new stars and planets?

The conservation of angular momentum in a Supernova can influence the formation of new stars and planets in several ways. The rotation of the debris from the explosion can lead to the formation of a disk, which can eventually coalesce into a new star or planets. Additionally, the angular momentum of the star's core can determine the type of Supernova and the resulting elements that are dispersed into space.

5. Is angular momentum always conserved in a Supernova?

While angular momentum is generally conserved in a Supernova, there may be cases where it is not. For example, if the star is rotating extremely fast or has a significant magnetic field, the conservation of angular momentum may be disrupted. Additionally, external forces, such as the gravitational pull of nearby objects, can also affect the conservation of angular momentum.

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