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In standard cosmology, comoving distance and proper distance (or physical distance) are two closely related distance measures used by cosmologists to define distances between objects. Comoving distance factors out the expansion of the universe, giving a distance that does not change in time except due to local factors, such as the motion of a galaxy…
Standards, Comoving distance and proper distance & Comoving coordinates
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distance comoving proper time universe coordinate expansion observers relativity light displaystyle two coordinates distances frame cosmological measured physical local would
| Subject | Predicate | Object | Confidence | Src |
|---|---|---|---|---|
| stars | instance of | in which the local speed of light is c and in which massive objects | 0.80 | text |
| galaxies always have a local speed smaller than c | instance of | in which the local speed of light is c and in which massive objects | 0.80 | text |
| Comoving and proper distances | related to Uses of the proper distance | Cosmological | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | Proper | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | To | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | All | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | Each | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | It | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | For | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | Comoving | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | This | 0.60 | section |
| Comoving and proper distances | related to Uses of the proper distance | When | 0.60 | section |
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