그림:Redrosedust wright f2000.jpg
위키백과 ― 우리 모두의 백과사전.
[edit] Summary
| Description |
English: A close up view of the Rosette Nebula. The red color comes from Hydrogen.
Français : Gros plan de la nébuleuse Rosette. La couleur rouge vient de l'hydrogène
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|---|---|
| Source |
http://astro.ic.ac.uk/Research/Halpha/North/gallery.shtml - accessed 5/07,2007 |
| Date |
05/07/2007 |
| Author |
English: Image based on data obtained as part of the INT Photometric H-Alpha Survey of the Northern Galactic Plane, prepared by Nick Wright, University College London, on behalf of the IPHAS Collaboration
Français : Image basée sur des données acquises lors de la cartographie H-alpha du plan galactique nord par l'INT, préparée par Nick Wright, University College London, dans le cadre de la collaboration IPHAS.
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| Permission (Reusing this image) |
Disclaimer: These images are released into the public domain for private use or for use in the promotion of the IPHAS survey. If any image or images are redisplayed or reproduced, please accompany the image or images with the following acknowledgement: "Image based on data obtained as part of the INT Photometric H-Alpha Survey of the Northern Galactic Plane, prepared by Nick Wright, University College London, on behalf of the IPHAS Collaboration". |
[edit] Licensing
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This file has been (or is hereby) released into the public domain by its author, INT Photometric Hα Survey of the Northern Galactic Plane - Nick Wright, University College London. This applies worldwide.
In case this is not legally possible: العربية | Български | Česky | Dansk | Deutsch | Ελληνικά | English | Español | فارسی | Français | Italiano | 日本語 | Nederlands | Polski | Português | Русский | Svenska | Türkçe | Українська | 中文 | 中文(台灣) | +/- |
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This file was a candidate on Picture of the Year 2006. This is a featured picture on Wikimedia Commons: it is considered one of our finest images. If you have an image of similar quality that can be published under a suitable copyright license, be sure to upload it, tag it, and nominate it. |
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This image was selected as a picture of the day for October 30, 2007. It was captioned as followed:
English: A better close up view of the Rosette Nebula. The red color comes from Hydrogen.
Deutsch: Eine Nahaufnahme des Rosettennebels. Die rote Farbe kommt vom Wasserstoff.
English: A better close up view of the Rosette Nebula. The red color comes from Hydrogen.
Español: Una imagen de la Nebulosa Roseta. El color rojo proviene del hidrógeno.
Français : Gros plan de la nébuleuse Rosette. La couleur rouge est due de l'hydrogène.
Magyar: A Rozetta-köd, Tejútrendszerünk egyik H II régiójának képe. A köd vöröses színe a gerjesztett hidrogénatomok sugárzásából ered.
日本語: ばら星雲 (NGC2237-9,46)。赤色は水素に由来する。
Latina: Conspectus Nebulae Rosettae. Color ruber venit e Carbonio.
Polski: Zbliżenie mgławicy Rosette. Kolor czerwony wskazuje na obecność wodoru.
Português: Uma imagem de perto da Nebulosa da Roseta. A cor vermelha é proveniente do Hidrogênio.
Српски / Srpski: Велики приказ небуле Розете. Црвена боја потиче од хидрогена.
Svenska: Närbild av Rosettnebulosan.
中文(简体): 麒麟座的蔷薇星云（NGC 2244），红色是水分子造成的。
中文(繁體): 玫瑰星雲（NGC 2237）的特寫照，星雲的紅色結構由氫分子構成
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파일 역사
날짜/시간을 누르면 당시의 파일을 볼 수 있습니다.
| 날짜/시간 | 크기 | 사용자 | 내용 | |
|---|---|---|---|---|
| 현재 | 2007년 5월 8일 (화) 03:10 | 5,388×3,777 (3.51 MB) | Clh288 | |
| 2006년 11월 22일 (수) 09:31 | 2,000×1,402 (442 KB) | Xixtas | ({{Information |Description=A close up view of the Rosette Nebula. The red color comes from Hydrogen. |Source=http://antwrp.gsfc.nasa.gov/apod/ap051223.html - accessed 11/21,2006 |Date= 11/21/2006 |Author= NASA |Permission= US Government. |other_versions= ) |
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| Orientation | Normal |
|---|---|
| Horizontal resolution | 71 dpi |
| Vertical resolution | 71 dpi |
| Software used | Adobe Photoshop Elements 2.0 |
| File change date and time | 2005년 11월 11일 (금) 13:35 |
| Color space | 65535 |
