File:Angular-size-redshift-relation.png
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Summary
| Description | The angular size redshift relation for a Lambda cosmology. This shows how the number of kiloparsecs per arcsecond changes with redshift. Note that after a redshift of about 1.5, objects appear larger with increasing distance. This was calculated using the web page of E. L. Wright http://www.astro.ucla.edu/~wright/CosmoCalc.html |
| Date | 2 April 2006 (original upload date) |
| Source | No machine-readable source provided. Own work assumed (based on copyright claims). |
| Author | No machine-readable author provided. Hjb26 assumed (based on copyright claims). |
Licensing
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I, the copyright holder of this work, release this work into the public domain. This applies worldwide. In some countries this may not be legally possible; if so: I grant anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law. |
File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 13:01, 2 April 2006 | | 400 × 269 (12 KB) | wikimediacommons>Hjb26 | The en:angular size redshift relation for a Lambda cosmology This shows how the number of kiloparsecs per arcsecond changes with redshift. Note that after a redshift of about 1.5, objects appear ''larger'' with increasing |
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