File:Optical parallax.jpg
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Optical_parallax.jpg (640 × 170 pixels, file size: 16 KB, MIME type: image/jpeg)
Summary
This drawing illustrates how north and south observers how image the Venus transit from the same longitude line should see the Venus's disk in two different places on the face of the Sun. The distance to the Sun is measurable directly and optically - without using clock based formulas.
Copyright status
Released to the Public
Source
Victor McAllister - author of this article.
File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 08:19, 8 November 2008 | | 640 × 170 (16 KB) | Victormc (talk | contribs) | This drawing illustrates how north and south observers how image the Venus transit from the same longitude line should see the Venus's disk in two different places on the face of the Sun. The distance to the Sun is measurable directly and optically - with |
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