File:Optical parallax.jpg

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Optical_parallax.jpg ‎(640 × 170 pixels, file size: 16 KB, MIME type: image/jpeg)

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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.

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Date/TimeThumbnailDimensionsUserComment
current08:19, 8 November 2008Thumbnail for version as of 08:19, 8 November 2008640 × 170 (16 KB)VictormcThis 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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