Sources
Help build the largest human-edited directory on the web.
Submit a site - Become an editor
Wikipedia. Licensed under the GNU Free Documentation License.
Are you an expert in this subject? Join the discussion and share your knowledge at Wikipedia.org.
Cosmological horizon
From Wikipedia, the free encyclopedia
| Physical Cosmology |
 |
| Physical Cosmology |
|
Universe · Big Bang |
| Early universe |
| Expanding universe |
|
Redshift · Hubble's law |
| Structure formation |
|
Shape of the universe |
| Components |
| History |
| Cosmology experiments |
| Scientists |
|
Einstein · Lemaître · Friedman |
|
|
In physical cosmology, a cosmological horizon marks a limit to observability, and marks the boundary of a region that an observer cannot see into directly due to cosmological effects.
The existence, properties, and significance of a cosmological horizon depend on the particular cosmological model being discussed.
In any case, it is interesting to note that the cosmological horizon is a maximal limit of perception and not an actual boundary. Much like an individual who is unable to see the edges of the Pacific Ocean while they are floating in the middle of it; we can only see the light from areas of space within the cosmological horizon.
This is sometimes referred to as the “observable universe”, and it has been said that the observable universe is many orders of magnitude smaller than the greater universe that lies beyond the limits of our perception.
Imagine if you will, that the entire cosmological horizon were reduced down to the size of quarter. If Alan Guth's inflationary model of early era cosmology is correct, the universe that lies beyond this “quarter sized” horizon would conservatively be as large as the earth itself.
 |
This physics-related article is a stub. You can help Wikipedia by expanding it. |