File:1911 Britannica - Astronomy - Practical.png
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1911_Britannica_-_Astronomy_-_Practical.png (514 × 174 pixels, file size: 24 KB, MIME type: image/png)
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[edit]Description1911 Britannica - Astronomy - Practical.png |
English: Practical Astronomy. PO (left fig.) is the direction of a ray, either from a heavenly body or from a terrestrial point, impinging at O upon the surface of quicksilver, and reflected in the direction OR, the vertical line is the bisector OZ, of the angle POR. If the point P is so adjusted over the quicksilver that the ray is reflected back on its own path, P and R lying on the same line above O, then we know that the line PO is truly vertical. The zenith-distance of an object is the angle which the ray of light from it makes with the vertical direction thus defined. To show the principle involved in the spirit-level let MN (right fig.) be the tube of such a level, fixed to an axis OZ on which it may revolve. If this axis is so adjusted that in the course of a revolution around it the bubble of the level undergoes no change of position, we know that the axis is truly vertical. Illustration from 1911 Encyclopædia Britannica, article Astronomy. |
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Encyclopædia Britannica Eleventh Edition, Vol. 2, Page 807 ![]() |
Author | Encyclopædia Britannica, 1911 |
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This image comes from the 13th edition of the Encyclopædia Britannica or earlier. The copyrights for that book have expired in the United States because the book was first published in the US with the publication occurring before January 1, 1929. As such, this image is in the public domain in the United States. | ![]() |
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