File:Dragonfish600.jpg

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描述

This infrared image from NASA's Spitzer Space Telescope shows the nebula nicknamed "the Dragonfish." This turbulent region, jam-packed with stars, is home to some of the most luminous massive stars in our Milky Way galaxy. It is located approximately 30,000 light-years away in the Crux constellation.

The massive stars have blown a bubble in the gas and dust, carving out a shell of more than 100 light-years across (seen in lower, central part of image). This shell forms the "toothy mouth" of the Dragonfish, and the two bright spots make it up its beady eyes.

The infrared light in this region is coming from the gas and dust that are being heated up by the unseen central cluster of massive stars. The bright spots along the shell, including the "eyes," are possible smaller regions of newly formed stars, triggered by the compression of the gas and dust by winds from the central, massive stars.

Infrared light in this image was captured by the infrared array camera on Spitzer, at wavelengths of 3.6 microns (blue); 4.5 microns (green); and 8.0 microns (red). The data were captured before Spitzer ran out of its liquid coolant in 2009, and began its "warm" mission.

日期

2011年12月12日

來源

http://www.spitzer.caltech.edu/images/4838-sig11-018-Dragonfish-Coming-At-You-in-Infrared (direct link)

作者

NASA/JPL-Caltech/Univ. of Toronto

授權許可
(重用此檔案)

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其他版本

This image is a JPEG version of the original TIFF image at File: Dragonfish nebula in infrared (captured by the Spitzer Space Telescope).tif.

This JPEG version should be used when displaying the file from Commons, as the MediaWiki software is unable to create a thumbnail or preview of the original TIFF file, because it is larger than 1000 megapixels. However, any edits to the image should be based on the original TIFF version in order to prevent generation loss, and both versions should be updated. Do not make edits based on this version.

檔案歷史

點選日期/時間以檢視該時間的檔案版本。

	日期/時間	縮⁠圖	尺寸	用戶	備⁠註
目前	2011年12月30日 (五) 15:47		7,600 × 5,500（26.37 MB）	Prof. Professorson	Higher resolution, from http://www.spitzer.caltech.edu/images/4838-sig11-018-Dragonfish-Coming-At-You-in-Infrared (http://www.spitzer.caltech.edu/uploaded_files/images/0008/4180/sig11-018.jpg).
	2011年1月26日 (三) 13:37		600 × 460（69 KB）	Shizhao	== {{int:filedesc}} == {{Information \|Description=Dragonfish nebula \|Source=http://www.newscientist.com/blogs/shortsharpscience/2011/01/dragonfish-nebula-conceals-gia.html \|Date=2011-01 \|Author=NASA/JPL-Caltech/GLIMPSE Team/M Rahman/U of Toronto \|Permissi

檔案用途

下列頁面有用到此檔案：

龍魚星雲

全域檔案使用狀況

以下其他 wiki 使用了這個檔案：

en.wikipedia.org 的使用狀況
en.wikiversity.org 的使用狀況
es.wikipedia.org 的使用狀況
- Nebulosa del Pez Dragón
tr.wikipedia.org 的使用狀況
- En büyük bulutsular listesi
vi.wikipedia.org 的使用狀況
- Tinh vân Long Ngư

詮釋資料

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如果此檔案的來源檔案已被修改，一些資訊在修改後的檔案中將不能完全反映出來。

影像標題	This infrared image from NASA's Spitzer Space Telescope shows the nebula nicknamed "the Dragonfish." This turbulent region, jam-packed with stars, is home to some of the most luminous massive stars in our Milky Way galaxy. It is located approximately 30,000 light-years away in the Crux constellation. The massive stars have blown a bubble in the gas and dust, carving out a shell of more than 100 light-years across (seen in lower, central part of image). This shell forms the "toothy mouth" of the Dragonfish, and the two bright spots make it up its beady eyes. The infrared light in this region is coming from the gas and dust that are being heated up by the unseen central cluster of massive stars. The bright spots along the shell, including the "eyes," are possible smaller regions of newly formed stars, triggered by the compression of the gas and dust by winds from the central, massive stars. Infrared light in this image was captured by the infrared array camera on Spitzer, at wavelengths of 3.6 microns (blue); 4.5 microns (green); and 8.0 microns (red). The data were captured before Spitzer ran out of its liquid coolant in 2009, and began its "warm" mission.
簡稱	Dragonfish Coming At You in Infrared
製作/提供者	NASA/JPL-Caltech/Univ. of Toronto
標題	This turbulent region, jam-packed with stars, is home to some of the most luminous massive stars in our Milky Way galaxy.
來源	Spitzer Space Telescope
使用條款	Public Domain
資料產生的日期時間	2011年12月12日 (星期一)
寬度	7,600 px
高度	5,500 px
每像素位元	8 8 8
壓縮方式	LZW
像素合成	RGB
方位	標準
像素數量	3
水平解析度	72 dpi
垂直解析度	72 dpi
資料排列	矮胖格式
使用軟體	Adobe Photoshop CS3 Macintosh
檔案修改日期時間	2011年12月12日 (一) 11:19
色彩空間	sRGB
聯絡資訊	http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA

File:Dragonfish600.jpg

說明

在此檔案描寫的項目

描繪內容

著作權狀態 ^{繁體中文 (已轉換拼寫)}

公有領域

成立或建立時間

12 12 2011

多媒體型式 ^{繁體中文 (已轉換拼寫)}

image/jpeg

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

File:Dragonfish600.jpg

說明

在此檔案描寫的項目

描繪內容

著作權狀態 繁體中文 (已轉換拼寫)

公有領域

成立或建立時間

12 12 2011

多媒體型式 繁體中文 (已轉換拼寫)

image/jpeg

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

著作權狀態 ^{繁體中文 (已轉換拼寫)}

多媒體型式 ^{繁體中文 (已轉換拼寫)}