Using the Hubble Telescope to Determine the Split of a Cosmological Object's Redshift in its Gravitational and Distance Parts: Difference between revisions
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{{Infobox paper | {{Infobox paper | ||
| title = Using the Hubble Telescope to Determine the Split of a Cosmological | | title = Using the Hubble Telescope to Determine the Split of a Cosmological | ||
Object | Object's Redshift in its Gravitational and Distance Parts | ||
| author = [[Pharis E Williams]] | | author = [[Pharis E Williams]] | ||
| keywords = [[gravitational redshift]], [[cosmological redshift]], [[Hubble telescope]], [[Weyl gauge factor]], [[gauge function]], [[unit of action]], [[variable unit of action]] | | keywords = [[gravitational redshift]], [[cosmological redshift]], [[Hubble telescope]], [[Weyl gauge factor]], [[gauge function]], [[unit of action]], [[variable unit of action]] | ||
Revision as of 23:41, 19 July 2026
| Scientific Paper | |
|---|---|
| Title | Using the Hubble Telescope to Determine the Split of a Cosmological Object's Redshift in its Gravitational and Distance Parts |
| Author(s) | Pharis E Williams |
| Keywords | gravitational redshift, cosmological redshift, Hubble telescope, Weyl gauge factor, gauge function, unit of action, variable unit of action |
| Published | 2001 |
| Journal | Apeiron |
| Volume | 8 |
| Number | 2 |
| No. of pages | 11 |
| Pages | 84-95 |
Abstract
The Hubble Telescope should make it possible to separate the redshift of light from any cosmological object into that redshift due to the gravitational potential difference between the emission and reception points and that portion due the distance between these points by comparing the redshifts measured on the Earth's surface to redshifts measured by the Hubble Telescope. This would allow a remapping of the cosmological objects and an increased understanding of gravitational conditions of these objects.