ملف:1e16m comparison 10 light years sirius.png
الملف الأصلي (1٬024 × 768 بكسل حجم الملف: 72 كيلوبايت، نوع MIME: image/png)
⧼wm-license-information-description⧽ |
English: Comparison of sizes of objects with order of magnitude 1e16m: ten light year radius shell with yellow Vernal Point arrow; below, white star Sirius 8.5 light years from Sun; on left, BL Ceti 8.73 light years distant; middle right, Proxima and Alpha Centauri about 4 light years distant; light year shell with Great January comet (Comet C/1910 A1)'s orbit shown as long extreme ellipse inside. All distances to scale, but stars are artificially enlarged for illustrative purposes only. No transparency version.
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⧼wm-license-information-date⧽ | 2008 |
⧼wm-license-information-source⧽ | derived from Paul Stansifer's POV-Ray source files (see below), by me, 84user, using w:en:POV-Ray, and w:en:IrfanView.
84user's contribution (inside POV-Ray files: adjusting coordinates, changing light source and other parameters) is public domain and source files used are described at User:84user/Size comparison. Physical information is based on the Wikipedia articles and elsewhere (see POVRay source files) about the respective lengths. Paul Stansifer's contributions to this image (POV-Ray code) are available under the GPL, v. 2, and other licenses. See User:Paul Stansifer/Size comparison for more details and the other licenses. |
⧼wm-license-information-author⧽ | Paul Stansifer, and User:84user (see "source") |
ترخيص
Because this image was rendered using only Paul Stanfiser's POV source code (no external texture maps used), it is a pure derivative. Therefore Paul's licenses apply; you may use it under the terms of any of these:
قالب:GPLv2 only قالب:GFDL-en قالب:CC-BY-SA-2.5
See also
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تاريخ الملف
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زمن/تاريخ | صورة مصغرة | الأبعاد | مستخدم | تعليق | |
---|---|---|---|---|---|
حالي | ★ مراجعة معتمدة 06:27، 28 نوفمبر 2023 | 1٬024 × 768 (72 كيلوبايت) | Pastakhov (نقاش | مساهمات) | Upload https://upload.wikimedia.org/wikipedia/commons/1/10/1e16m_comparison_10_light_years_sirius.png |
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