@OrCkHaNtheGrEaT This is the universe from our percpective, we are in the center. As we look further out into space, we see the universe as it was more time ago. You'll notice that as it comes further out the galaxies appear to be less formed, as they were many billions of years ago.
@nadoeloiskat I would really like an answer to this as well. I have a sense it is a projected hypotheses but due to scale in comparison to everything else contained within inclusive of dark matter, it would be really good to get a definite answer of just how big a universe we are currently aware of in terms of extremity.
This is a simulated view of the Universe from our point of view in space. The black areas are areas of the Universe that are blocked from our view because we're inside our own Galaxy. Imagine you're out in the countryside with clear skies but a thick ground fog.... you can look up and see the stars high in the sky, but the stars close to the horizon and nearby trees are obscured by fog. Same principle in looking at faraway galaxies.
@djxatlanta They can only observe a small portion of the time when they do this survey so basically they are taking slices of the sky each time and going deep into that area of slice. Now combining multiple slices would eventually lead to a full 3D image, however this takes a very long time thats why so far we have empty spaces. Also in the middle it should look more clogged up because as we go further away from the middle the telescope will be able to see less galaxies because its so far away
Does anyone claim to have an explanation why the distribution is the way it is? It appears like wings (or fans) emanating from a central point. Why is the distribution not simply even across space?
@wolverine005 - exactly right... it takes a LOT of time to precisely map each of these galaxies in space (and time), and we're nowhere close to being finished yet. Of course, because our own galaxy blocks the view of part of the universe, there will always be a gap.
@djxatlanta At least until we can get a different point of view that is. Fingers crossed we don't nuke the hell out of ourselves before that happens!!
@dhansen888 We know why the distrubition is like this. The initial conditions are provided by early universe inflation. The distribution is not even because of the quantum flutcutations in the early universe. The initial conditions are evolved in time according to the equations of General Relativity, resulting in this beautiful map. There is a mathematical way of decoding the information of the map, called a Fourier transform, and we can more easily compare the Fourier transform with theory.
it always amazes me.. ;-0
lovelplants 5 days ago
Why are there random gaps in the animation?
Jpwillerd 2 weeks ago
Wow, and people think we are alone in the universe.............
RodrogerAu 1 month ago
yellow region is the cosmic microwave background fluctuations?
ThemreEpi 1 month ago
why is the center of this map is more denser than the outer regions? shouldnt the universe has to be roughly the same density all around?
OrCkHaNtheGrEaT 2 months ago
@OrCkHaNtheGrEaT This is the universe from our percpective, we are in the center. As we look further out into space, we see the universe as it was more time ago. You'll notice that as it comes further out the galaxies appear to be less formed, as they were many billions of years ago.
jaykulls 1 month ago in playlist Liked videos
is this map made under visible light or combined frequencies? i mean would we see the same at the same distance to universe?
OrCkHaNtheGrEaT 2 months ago
Does anybody knows is this bubble in the end the entire estimated universe or the visible universe?
And is the estimated 100 billion galaxies in the visible or entire universe?
Or should i go to wikipedia for the answers?
nadoeloiskat 4 months ago
@nadoeloiskat I would really like an answer to this as well. I have a sense it is a projected hypotheses but due to scale in comparison to everything else contained within inclusive of dark matter, it would be really good to get a definite answer of just how big a universe we are currently aware of in terms of extremity.
nessusdawning 1 week ago
is that on a program that you can use,or is it only a video you can watch.
Akira89M 11 months ago
This is a simulated view of the Universe from our point of view in space. The black areas are areas of the Universe that are blocked from our view because we're inside our own Galaxy. Imagine you're out in the countryside with clear skies but a thick ground fog.... you can look up and see the stars high in the sky, but the stars close to the horizon and nearby trees are obscured by fog. Same principle in looking at faraway galaxies.
djxatlanta 2 years ago 11
This has been flagged as spam show
@djxatlanta They can only observe a small portion of the time when they do this survey so basically they are taking slices of the sky each time and going deep into that area of slice. Now combining multiple slices would eventually lead to a full 3D image, however this takes a very long time thats why so far we have empty spaces. Also in the middle it should look more clogged up because as we go further away from the middle the telescope will be able to see less galaxies because its so far away
Hosu223 2 days ago
Does anyone claim to have an explanation why the distribution is the way it is? It appears like wings (or fans) emanating from a central point. Why is the distribution not simply even across space?
dhansen888 2 years ago
@dhansen888 That's just area's we have yet to map. The gaps that is.
wolverine005 1 year ago 6
@wolverine005 - exactly right... it takes a LOT of time to precisely map each of these galaxies in space (and time), and we're nowhere close to being finished yet. Of course, because our own galaxy blocks the view of part of the universe, there will always be a gap.
djxatlanta 1 year ago
@djxatlanta At least until we can get a different point of view that is. Fingers crossed we don't nuke the hell out of ourselves before that happens!!
wolverine005 1 year ago 2
@dhansen888 We know why the distrubition is like this. The initial conditions are provided by early universe inflation. The distribution is not even because of the quantum flutcutations in the early universe. The initial conditions are evolved in time according to the equations of General Relativity, resulting in this beautiful map. There is a mathematical way of decoding the information of the map, called a Fourier transform, and we can more easily compare the Fourier transform with theory.
lfdmotta 1 year ago