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This thing you call with the Hubble light etc. Better explained it goes: It is called the >>>cosmic horizon<<< the maximum distance one cann see out into the universe at a given time. The horizon lies at a distance in light-years approximately equal to the age o the Universe in years. Haaha I know such stuff and i'm just 16 years old hihi
For galaxies relatively close to earth (small cosmological red shift) the red shift caused by the object's velocity can dominate over the red shift caused by the spacetime expansion (cosmological). So there's less scatter in Hubble's Law as you get further out because then the cosmological red shift is much greater and supercedes other effects.
Yeah I meant to mention something about how the magnitudes of red shift from various sources differ, But it got lost along the way damn my ADHD. I think I'll do a follow up on this one to explain how scientist determine redshift, I'll be sure to include it. Thanks for the input.
Good, glad I was able to answer your questions. I might do more of these, though I think I'll write atleast a loose script so I don't go all over the place like I did here.
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It is called the >>>cosmic horizon<<<
the maximum distance one cann see out into the universe at a given time. The horizon lies at a distance in light-years approximately equal to the age o the Universe in years.
Haaha I know such stuff and i'm just 16 years old hihi
For galaxies relatively close to earth (small cosmological red shift) the red shift caused by the object's velocity can dominate over the red shift caused by the spacetime expansion (cosmological). So there's less scatter in Hubble's Law as you get further out because then the cosmological red shift is much greater and supercedes other effects.
I'll be seeing you around.