Stellar and Planetary Aberration: Difference between revisions
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| journal = [[Apeiron]] | | journal = [[Apeiron]] | ||
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==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. | 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:Relativity]] | [[Category:Scientific Paper|stellar planetary aberration]] | ||
[[Category:Relativity|stellar planetary aberration]] | |||
Latest revision as of 09:23, 21 July 2026
| 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.