Relativistic mass increase due to high temperatures inside stars?

In summary, the core temperature of the Sun is 15.7×10^6 Kelvins according to Wikipedia. It is unknown if the protons' velocities inside the core have a noticeable increase in mass due to their relativistic speed. This could potentially influence the overall gravitational pull of a star and could be an explanation for dark matter. However, the protons move at a speed of ~0.1% of light speed, which does not contribute significantly to the star's mass. The Sun also sheds a small amount of mass every second due to its luminosity, but this is already taken into account in calculations of stellar mass. According to general relativity, both mass and energy contribute to gravity and are indistinguishable in
  • #1
kahoon
4
0
Wikipedia says that the core temperature of our Sun is 15.7×10^6 Kelvins.

I don't know what that means in terms of protons' velocities inside the core, but I bet they move pretty fast. Could they move that fast that they have a noticeable increase in mass due to their relativistic speed?

Could this influence the overall gravitational pull of a star?

Could this be an explanation for dark matter?
 
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  • #2
They move at ~0,1% light speed, that doesn't contribute noticeable to the star's mass. Maybe one part in a million.
 
  • #3
Because E=mc^2, a massive amount of energy is needed to resemble a small amount of mass both inertial and gravitational.

Let's look at how much mass the Sun "sheds" every second due to it's luminosity. The solar luminosity is 3.85*10^26W. That's equivalent of only 4.27*10^9kg/s. Considering the Sun's mass is 1.99*10^30kg, the mass of the sun is 21 orders of magnitude larger than the "luminosity mass". To be in equilibrium the Sun's energy production is roughly equal to the energy output (or else it would get hotter and hotter and eventually explode as all that energy built up!).

The other important point to note; however, is that this "mass" is already included in our calculations. We calculate the mass of massive stellar bodies from the orbits of objects orbiting them. We cannot tell if this gravitational mass is sourced by actual rest mass or by energy. In general relativity, both mass AND energy source gravity. To us, making these calculations, they are the same. We can't tell a shred of difference.
 

1. What is relativistic mass increase?

Relativistic mass increase, also known as mass-energy equivalence, is the phenomenon where the mass of an object increases as it moves at higher speeds. This is described by Einstein's famous equation E=mc², where E represents energy, m represents mass, and c represents the speed of light.

2. How does high temperature lead to relativistic mass increase?

According to the laws of thermodynamics, as the temperature of a system increases, so does its energy. This increase in energy leads to an increase in the mass of the system, as described by Einstein's equation. In stars, the high temperatures generated by nuclear fusion reactions cause an increase in the relativistic mass of the particles involved.

3. What role does the speed of particles play in relativistic mass increase?

The speed of particles is a crucial factor in relativistic mass increase. As particles move at higher speeds, their energy increases, causing an increase in their mass. This is why particles in accelerators, which can reach close to the speed of light, have a much higher relativistic mass than particles at rest.

4. Is there a limit to how much mass can increase due to high temperatures?

Yes, there is a limit to how much mass can increase due to high temperatures. The limit is the speed of light itself, as described by Einstein's equation. As an object approaches the speed of light, its mass increases infinitely, making it impossible to reach the speed of light.

5. How does relativistic mass increase affect the behavior of particles in stars?

The increase in mass due to high temperatures inside stars has a significant impact on the behavior of particles. It affects the rate of nuclear fusion reactions, as well as the pressure and density within the star. These factors ultimately determine the size, luminosity, and lifespan of a star.

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