
#1
Jun610, 07:45 AM

P: 59

Ignoring what we know. I was curious as to if anyone had overlayed all of the spectrum's of light on top of each other in a complete photonic view like the CMBR version, only with a much more varied scale, that being the entire light spectrum. And if so what did this produce? I only ask because I was thinking of Olber's shell model that he used in his paradox to decide whether or not the universe was infinite. And if this picture did or didn't produce an infinitely bright view, whether or not this would be sufficient evidence of the universe being infinite or not. Of course taking into account the flaws in his model, and also the time delay for photons of light to reach us since looking in particular at the CMBR, clearly large amounts of these photons are a lot older then those reaching us now.




#2
Jun610, 06:32 PM

P: 212

I don't know the answer to your specific question, but I think it's generally agreed that the distribution of matter through space is finite, but whether space it's self is infinite is probably open for debate.




#3
Jun810, 08:15 AM

P: 59

How can you tell if the distribution of matter throughout space is finite since you can't tell if there is anything beyond the light horizon of our universe, say another preexisting universe that isn't running parallel?




#4
Jun810, 08:35 AM

Sci Advisor
HW Helper
P: 8,961

complete photonic view like the CMBR version
The observable universe is finite (about 90Bn lyr accross) with a finite amount of matter in it.
whats beyond the obsevable universe doesn't matter 



#5
Jun810, 08:43 AM

P: 59

Well yea, but how do you know that the universe expands with the event horizon and doesn't go beyond it? And therefore there is something, anything, beyond that horizon that is undetectable to us? Saying "what's beyond it doesn't matter" isn't exactly helpful if say it can enter back across to our side of the horizon?




#6
Jun810, 08:58 AM

Mentor
P: 14,433





#7
Jun810, 09:04 AM

P: 59

Ahh ok that makes much more sense. Thanks D H



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