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Physics, Astronomy & Cosmology / Re: What happens when photons leave the sun?
« on: Today at 00:39:01 »Quote from: OP
how much Doppler shift is there?Each year, around 3-4th January (perihelion, closest to the Sun) and 3-4th July (aphelion, farthest from the Sun), the Earth is neither moving towards or away from the Sun, and there is no Doppler shift. Around October there is a maximum Doppler blue shift (Earth moving towards the Sun) and around May there is a maximum Doppler red shift (Earth moving away from the Sun).
As others have pointed out, all year long there is a gravitational red shift (or "Einstein shift"), as photons "climb out" of the Sun's gravitational well. Depending on your frame of reference, you could say some of the following things:
- Photons don't lose speed as they always travel at c
- Photons don't lose kinetic energy, since the photon is massless
- Photons do lose momentum
- The photon frequency does decrease
One way of looking at this frequency decrease is to consider Einstein's time dilation.
- Deep in a gravitational well (eg the surface of the Sun), time moves more slowly, compared to an observer on the surface of the Earth
- So a Hydrogen atom emitting a spectral line on the surface of the Sun will do so more slowly than a Hydrogen atom emitting the same spectral line on the surface of the Earth
- So when you compare the frequency of the light from the Sun with the frequency of light generated here on Earth, you will find the light from the Sun has a lower frequency.
Einstein shift will be a maximum at aphelion, and minimum at perihelion.
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photons are on their 1,000,000 year journey out of our sunUnder the extreme conditions of a supernova, energy from the core of a star can reach the surface much more quickly - just 3 to 4 hours.
But neutrinos don't interact much with matter; traveling at (pretty much) the speed of light, they can reach the surface of the star in just 1 second.
- To date, such a "race" has only been observed once, when a supernova occurred in the nearby Large Magellanic Cloud (a dwarf galaxy orbiting our Milky Way galaxy).
https://en.wikipedia.org/wiki/SN_1987A#Neutrino_emissions