File:Transit diagram angles-ar.png
Transit_diagram_angles-ar.png (441 × 295 pixels, file size: 15 KB, MIME type: image/png)
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Summary
editDescriptionTransit diagram angles-ar.png |
العربية: رسم يُظهر كيفيّة عبور الزهرة أمام قرص الشمس ولمَ لا تتكرر هذه الظاهرة غالبًا. |
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This file was derived from: Transit diagram angles.png: ![]() |
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This is a retouched picture, which means that it has been digitally altered from its original version. Modifications: translated to Arabic. The original can be viewed here: Transit diagram angles.png: ![]()
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This licensing tag was added to this file as part of the GFDL licensing update.http://creativecommons.org/licenses/by-sa/3.0/CC BY-SA 3.0Creative Commons Attribution-Share Alike 3.0truetrue |
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Permission is granted to copy, distribute and/or modify this document under the terms of the GNU Free Documentation License, Version 1.2 or any later version published by the Free Software Foundation; with no Invariant Sections, no Front-Cover Texts, and no Back-Cover Texts. A copy of the license is included in the section entitled GNU Free Documentation License.http://www.gnu.org/copyleft/fdl.htmlGFDLGNU Free Documentation Licensetruetrue |
Original upload log
editThis image is a derivative work of the following images:
- File:Transit_diagram_angles.png licensed with Cc-by-sa-2.5, Cc-by-sa-3.0-migrated, GFDL
- 2007-03-16T02:16:20Z Kjetil r 441x295 (9938 Bytes) {{Information |Description=Diagram showing how [[:en:transit of Venus|transits of Venus]] occur and why they don't occur frequently. Drawn by [[:en:User:Theresa Knott]]; License see: [http://en.wikipedia.org/w/index.php?title
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 16:42, 1 August 2012 | ![]() | 441 × 295 (15 KB) | باسم (talk | contribs) | == {{int:filedesc}} == {{Information |Description={{ar|رسم يُظهر كيفيّة عبور الزهرة أمام قرص الشمس ولمَ لا تتكرر هذه الظاهرة غالبًا. رُسمت الخريطة ... |
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Horizontal resolution | 35.43 dpc |
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Vertical resolution | 35.43 dpc |
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