File:HipparchusEclipse.png
HipparchusEclipse.png (486 × 280 pixels, file size: 6 KB, MIME type: image/png)
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La bildo estas kopiita de wikipedia:en. La originala priskribo estas:
Summary
Diagram used in reconstructing one of Hipparchus' methods of determining the distance to the moon. This represents the earth-moon system during a partial solar eclipse at A (Alexandria) and a total solar eclipse at H (Hellespont). Adapted from an image in Toomer 1974, p. 132. See Hipparchus On Sizes and Distances for full reference.
Licensing
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I, the copyright holder of this work, release this work into the public domain. This applies worldwide. In some countries this may not be legally possible; if so: I grant anyone the right to use this work for any purpose, without any conditions, unless such conditions are required by law. |
| date/time | username | edit summary |
|---|---|---|
| 06:49, 25 December 2005 | en:User:Dantheox | (Diagram used in reconstructing one of <a href="/wiki/Hipparchus" title="Hipparchus">Hipparchus'</a> methods of determining the distance to the <a href="/wiki/Moon" title="Moon">moon</a>. This represents the earth-moon system during a partial solar eclipse at A (<a href="/wiki/Alexandria" title="Alexandria">Alexandria</a>) and a total solar eclipse at H (<a href="/wiki/Hellespont" title="Hellespont">Hellespont</a>) |
Original upload log
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- (del) (cur) 06:49, 25 December 2005 . . en:User:Dantheox Dantheox ( en:User_talk:Dantheox Talk) . . 486x280 (6386 bytes) (Diagram used in reconstructing one of en:Hipparchus Hipparchus' methods of determining the distance to the en:Moon moon. This represents the earth-moon system during a partial solar eclipse at A ( en:Alexandria Alexandria) and a total solar eclipse at H ( en:Hellespont Hellespont)
File history
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| Date/Time | Thumbnail | Dimensions | User | Comment | |
|---|---|---|---|---|---|
| current | 21:05, 18 March 2006 | | 486 × 280 (6 KB) | Maksim | La bildo estas kopiita de wikipedia:en. La originala priskribo estas: == Summary == Diagram used in reconstructing one of Hipparchus' methods of determining the distance to the moon. This represents the earth-moon system during a parti |
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