Edithistory:De Vaucouleurs system
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| oldid | date/time | username | edit summary |
|---|---|---|---|
| 1369615462 | 2026-08-16T02:05:18Z | Ldm1954 | [[WP:AFC|AFC]] draft |
| 1369615453 | 2026-08-16T02:05:16Z | Ldm1954 | Ldm1954 moved page [[De Vaucouleurs system]] to [[Draft:De Vaucouleurs system]]: [[WP:DRAFTIFY|Not ready]] for mainspace, incubate in draftspace. Reason/s: machine-generated |
| 1369613704 | 2026-08-16T01:52:58Z | Ldm1954 | Added tags to the page using [[Wikipedia:Page Curation|Page Curation]] (ai-generated) |
| 1369463004 | 2026-08-15T03:51:41Z | Kadesthetics | 2 |
| 1368736917 | 2026-08-10T20:23:50Z | Frap | MOS:HEAD |
| 1368655669 | 2026-08-10T09:22:24Z | Mariamnei | Added tags to the page using [[Wikipedia:Page Curation|Page Curation]] (no footnotes) |
| 1368646119 | 2026-08-10T07:17:32Z | Kadesthetics | [[WP:AES|←]]Created page with '{{Short description|Galaxy morphological classification system}} {{Use dmy dates|date=December 2025}} The '''de Vaucouleurs system''', also known as the '''revised Hubble system''' or the '''de Vaucouleurs–Sandage system''', is a comprehensive [[galaxy morphological classification]] scheme developed by French astronomer [[Gérard de Vaucouleurs]] in 1959. It extends [[Edwin Hubble]]'s original [[Hubble sequence|tuning-fork classification]] into a three-d...' |
