Difference between revisions of "Stellar and Planetary Aberration"
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− | 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. |
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+ | [[Category:Scientific Paper|stellar planetary aberration]] | ||
[[Category:Relativity]] | [[Category:Relativity]] |
Revision as of 11:06, 1 January 2017
Scientific Paper | |
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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.