Energy and momentum flux in the sun and Newton's 3rd law.

In summary, Newton's Third Law states that for every action there is an equal and opposite reaction. In the case of the Sun, the photons traveling outward cause a recoil in the ions and electrons, but they quickly bump into each other and their initial inwards vector is randomized. Though there is an inwards pressure caused by the departing photons and solar wind, it is overshadowed by gravity's much larger influence.
  • #1
Spinnor
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Newton's Third Law of Motion:

III. For every action there is an equal and opposite reaction.

Photons in the sun on average travel outward, electrons and ions on average recoil inwards? Does Newton's third law come into play here?


Thank you for help with my confusion.
 
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  • #2
Electrons and ions on average recoil inwards? Actually, the Sun is a net producer of charged particles; this stream of particles is called the solar wind.

It's true that Newton's third law (and its corollary, the conservation of momentum) apply to the fusion reacts that produce photons, but it's not as if those photons are streaming out into space. The gamma photons produced enter the convection zone, where energy transfer is mostly via convection. The photons we see are black-body photons produced very near the surface of the Sun, not the gamma photons produced by fusion reactions.
 
  • #3
Correct-ish

Spinnor said:
Newton's Third Law of Motion:

III. For every action there is an equal and opposite reaction.

Photons in the sun on average travel outward, electrons and ions on average recoil inwards? Does Newton's third law come into play here?


Thank you for help with my confusion.

You're right to suspect that the ions and electrons throwing off photons from the Sun's photosphere experience a recoil from Newton's 3rd law. However they're very rapidly bumping into other ions and electrons before they travel very far in the photosphere, so any initially inwards vector is soon randomised.

The photons - and, to a lesser extent, the solar wind - do cause an inwards pressure in reaction to their departure, but that's overwhelmed by gravity's much greater hold on them. The Sun would need to be much, much hotter and brighter for light pressure to match gravity in the photosphere.
 

1. What is the main source of energy in the sun?

The main source of energy in the sun is nuclear fusion, which occurs in its core. This process involves the fusion of hydrogen atoms to form helium, releasing a large amount of energy in the process.

2. How does energy and momentum flux contribute to the sun's stability?

The high energy and momentum flux within the sun's core help to maintain its stability by counteracting the gravitational force pulling inwards. This creates a balance between the outward pressure and inward pull, preventing the sun from collapsing on itself.

3. How is the energy and momentum flux in the sun related to Newton's 3rd law?

According to Newton's 3rd law, for every action, there is an equal and opposite reaction. In the case of the sun, the high energy and momentum flux generated by nuclear fusion in its core create a force that pushes outward, and this is balanced by an equal and opposite force pulling inward due to gravity.

4. How does the sun's energy and momentum flux affect other objects in the solar system?

The energy and momentum flux from the sun play a crucial role in the dynamics of the entire solar system. The sun's gravitational pull and its energy output affect the orbit and movement of all the planets, moons, and other objects in the solar system.

5. Can we measure the energy and momentum flux in the sun?

Yes, scientists use various methods to measure the energy and momentum flux in the sun, such as observing solar radiation, analyzing solar winds, and studying the movements of objects in the solar system. These measurements help us understand the sun's dynamics and its impact on the entire solar system.

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