Why Do We Experience Night in Our Universe?

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Discussion Overview

The discussion centers around the question of why we experience night in the universe, exploring various theories and concepts related to cosmology, including Olber's paradox, the finite age of the universe, and the effects of cosmic expansion and dark matter.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that the universe's expanding rate may be faster than light, preventing visible light from reaching Earth.
  • Others reference Olber's paradox, noting that the finite age of the universe means light from distant stars has not had time to reach us.
  • There are claims that dark matter could absorb light, contributing to the darkness of the night sky, though this is debated.
  • One participant argues that while light intensity decreases with distance, the number of stars in a given viewing angle increases, suggesting that this does not fully explain the darkness.
  • Another point raised is that the cosmic microwave background radiation is the oldest observable light, and before that, the universe was opaque.
  • Some participants discuss the implications of the universe's finite extent and the cosmological horizon on our ability to observe stars and galaxies.
  • There are questions about whether the universe is expanding faster than the speed of light and how this relates to the visibility of distant objects.
  • Concerns are raised about the validity of assuming a finite age for the universe, with references to ongoing research that explores conditions before the Big Bang.
  • One participant highlights that as the universe expands, we may eventually observe less light, leading to a future where the night sky is completely dark.

Areas of Agreement / Disagreement

Participants express multiple competing views regarding the causes of night, with no consensus reached on the primary factors contributing to the darkness of the night sky. Disagreements exist about the implications of cosmic expansion, the nature of dark matter, and the assumptions regarding the universe's age and extent.

Contextual Notes

Some claims depend on definitions of terms like "finite" and "infinite," and there are unresolved questions about the mathematical models used to describe the universe's behavior before the Big Bang. The discussion also touches on the limitations of current observational capabilities due to the cosmological horizon.

  • #31
Nabeshin said:
I like you :smile:

Quote again I did get get the "orbit" and "rotate" mixed up.
Excuse me for that.

-Derek
 
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  • #32
Its simple. We have night because the Earth rotates away from the Sun. The sun's light only takes 8 minutes to get to Earth. Other stars produce light otherwise we would never see them. Those stars are just so much farther away than the sun that the light does not have as much of an effect. The Earth is always getting hit with light, its just not strong enough to produce day like the sun does.
 
  • #33
Saturni, GetPhysical, it doesn't appear that either of you actually read the OP. The title doesn't specify that it is discussing Obler's paradox, but the post itself clearly does (without using the name). The title should probably say - "Why is the night sky not as bright as the sun?", which is the question Obler's paradox asks.
 
  • #34
marcus said:
So there is currently no scientific reason to assume that the universe has a finite age.

There is conversely no scientific reason to assume that the universe has an infinite age.

Yes, universe-models can be projected out to times before the big bang, but this isn't necessarily an accurate projection. Furthermore, what if there was a bigger, more grandiose "starter-event" beyond which there really WAS nothing? (like a big-bang before the big-bang)
 
  • #35
We have night so we can sleep. We have day so we can wake up. Wes Hughes
 
  • #36
JesseM said:
I think you're talking about Olber's paradox. Expansion plays some role, but the main thing to keep in mind is that the universe is thought to have only a finite age, so light from stars too far away just won't have had time to reach us.

If the universe is 14.5 billion years old and If some stars are so far away they haven't had time to reach us yet wouldn't that mean that the universe was at least 14.5 billion ly wide when it was formed. and if the universe was created with a big bang it would have had to expand awfully fast to get to 14.5 b ly wide before any stars formed to start emitting light. also if we look far enough away shouldn't we stop seeing galaxies and start seeing just stars if the universe was created by a big bang and stars formed first and then the stars formed into galaxies?
 
  • #37
discord73 said:
If the universe is 14.5 billion years old and If some stars are so far away they haven't had time to reach us yet wouldn't that mean that the universe was at least 14.5 billion ly wide when it was formed. and if the universe was created with a big bang it would have had to expand awfully fast to get to 14.5 b ly wide before any stars formed to start emitting light. also if we look far enough away shouldn't we stop seeing galaxies and start seeing just stars if the universe was created by a big bang and stars formed first and then the stars formed into galaxies?

Ok, I wrote out some stuff on this then accidentally navigated away and lost it all. So you are going to have to seek out the references yourself, because frankly I can't be bothered doing it again.

The observable universe is 46.5 billion ly in radius. The age of the universe is 13.73 billion years (give or take a bit). The earliest radiation we can see is CMB, which is about 3.35 billion years old. The actual size of the universe is thought to be at least 78 billion ly in radius. So your figures are out.

You have misunderstood how cosmological expansion works (not to mention star and galaxy formation).

Here are some figures which may help. The rate at which two points in space expand due to cosmological expansion is proportional to their separation (multiplied by the Hubble constant).

Alpha Centauri is 4.37 ly away, so we are separating from AC at 1mm/s. When light reaches us from AC, we have separated by about 30 km.

Omega Farus (I made it up) was 3.5 billion light years away when a photon was emitted. Once that photon has traveled 3.5 billion light years, assuming an invariant Hubble constant at its current value, then the separation (between the source and us) will have increased by about 1.5 billion light years. Note, this is hugely simplified - for example, 3.5 billion years ago the Hubble constant would have been about a third again more than what it is now, which means that we and Omega Farus were separating more quickly when the photon started out but on the other hand, the rate of separation between where the photon was and where we were would decrease as the photon approached us. The point is that a photon from a star that was 3.5 billion ly away at emission would take (very very roughly, assuming a Hubble constant of 70.8 throughout and doing some very rough element analysis) about 5 billion years to get to us.

I'm sure there is someone else out there who has done the more complicated maths :)

cheers,
neopolitan
 
  • #38
marcus said:
Is thought by whom? A lot of the research going on in modern cosmology extends the models back before the big bang.
While that may be true, I do believe that, by definition, our universe began with the BB. Whatever was before the BB is not part of this universe.
 
  • #39
it seems that there are grounds for saying that the "edge of the universe" is expanding away from us at the speed of light, if we define the edge of the universe to be "that bounding everything that can or ever could have an impact on us" - it's not necessarily a real thing. Since the edge of the universe is 14 billion light years and the universe is suspiciously close to 14 billion years old.http://www.o2sensorsdirect.com"
 
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