Difference between revisions of "Stellar and Planetary Aberration"
Jump to navigation
Jump to search
(Imported from text file) |
(Imported from text file) |
||
| Line 12: | Line 12: | ||
==Abstract== | ==Abstract== | ||
| − | A way of looking at the topics of stellar and planetary aberration is suggested that enables them to be viewed as closely related?both being conceived as dependent on source-detector relative velocity. We show that the long-range limiting case, stellar aberration, has certain uniquely subtle aspects, as well as some hypothesized characteristics that lend themselves to empirical testing.[[Category:Scientific Paper]] | + | A way of looking at the topics of stellar and planetary aberration is suggested that enables them to be viewed as closely related?both being conceived as dependent on source-detector relative velocity. We show that the long-range limiting case, stellar aberration, has certain uniquely subtle aspects, as well as some hypothesized characteristics that lend themselves to empirical testing. |
| + | |||
| + | [[Category:Scientific Paper|stellar planetary aberration]] | ||
[[Category:Relativity]] | [[Category:Relativity]] | ||
Revision as of 11:06, 1 January 2017
| Scientific Paper | |
|---|---|
| Title | Stellar and Planetary Aberration |
| Author(s) | Thomas E Phipps |
| Keywords | planetary aberration, stellar aberration |
| Published | 1994 |
| Journal | Apeiron |
| Volume | 1 |
| No. of pages | 7 |
| Pages | 12-18 |
Abstract
A way of looking at the topics of stellar and planetary aberration is suggested that enables them to be viewed as closely related?both being conceived as dependent on source-detector relative velocity. We show that the long-range limiting case, stellar aberration, has certain uniquely subtle aspects, as well as some hypothesized characteristics that lend themselves to empirical testing.
