File:A giant, smouldering star.jpg

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摘要

描述A giant, smouldering star.jpg	English: This new image, snapped by NASA/ESA Hubble Space Telescope, shows the star HD 184738, also known as Campbell’s hydrogen star. It is surrounded by plumes of reddish gas — the fiery red and orange hues are caused by glowing gases, including hydrogen and nitrogen. HD 184738 is at the centre of a small planetary nebula. The star itself is known as a [WC] star, a rare class resembling their much more massive counterparts — Wolf-Rayet stars. These stars are named after two French astronomers, Charles Wolf and Georges Rayet, who first identified them in the mid-nineteenth century. Wolf-Rayet stars are hot stars, perhaps 20 times more massive than the Sun, that are rapidly blowing away material and losing mass. [WC] stars are rather different: they are low-mass Sun-like stars at the end of their lives. While these stars have recently ejected much of their original mass, the hot stellar core is still losing mass at a high rate, creating a hot wind. It is these winds that cause them to resemble Wolf-Rayet stars. However, astronomers can look more closely at the composition of these winds to tell the stars apart; [WC] stars are identified by the carbon and oxygen in their winds. Some true Wolf-Rayet stars are rich in nitrogen instead, but this is very rare among their low-mass counterparts. HD 184738 is also very bright in the infrared part of the spectrum, and is surrounded by dust very similar to the material that the Earth formed from. The origin of this dust is uncertain. A version of this image was entered into the Hubble’s Hidden Treasures image processing competition by contestant Jean-Christophe Lambry.
日期	2013年9月16日, 10:00:00
來源	http://www.spacetelescope.org/images/potw1337a/
作者	ESA/Hubble & NASA Acknowledgement: Jean-Christophe Lambry

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	日期/時間	縮⁠圖	尺寸	使用者	備⁠註
目前	2019年12月31日 (二) 09:15		501 × 501（86 KB）	BevinKacon	actual size from source
	2013年9月17日 (二) 00:49		1,280 × 1,280（178 KB）	Jmencisom	User created page with UploadWizard

檔案用途

下列2個頁面有用到此檔案：

全域檔案使用狀況

以下其他 wiki 使用了這個檔案：

ast.wikipedia.org 的使用狀況
- Estrella de Campbell
ca.wikipedia.org 的使用狀況
- Estrella de Campbell
en.wikipedia.org 的使用狀況
- Wolf–Rayet star
es.wikipedia.org 的使用狀況
- Cygnus (constelación)
- Estrella de Campbell
eu.wikipedia.org 的使用狀況
- Wolf-Rayet izar
fr.wikipedia.org 的使用狀況
- Discussion:Listes de nébuleuses planétaires
it.wikipedia.org 的使用狀況
- Stella di Wolf-Rayet
- Stella di Campbell
ko.wikipedia.org 的使用狀況
- 볼프–레이에별
mk.wikipedia.org 的使用狀況
- BD+30 3639
- Волф-Рајеова ѕвезда
pt.wikipedia.org 的使用狀況
- Estrela Wolf-Rayet
ru.wikipedia.org 的使用狀況
- Портал:Астрономия/Изображение недели 2013
sk.wikipedia.org 的使用狀況
- Wolfova-Rayetova hviezda
sr.wikipedia.org 的使用狀況
- Volf-Rajeova zvezda
www.wikidata.org 的使用狀況
- Q5849651

詮釋資料

此檔案中包含其他資訊，這些資訊可能是由數位相機或掃描器在建立或數位化過程中所新增的。若檔案自原始狀態已被修改，一些詳細資料可能無法完整反映出已修改的檔案。

來源	ESA/Hubble
製作/提供者	ESA/Hubble & NASA Acknowledgement: Jean-Christophe Lambry
影像標題	This new image, snapped by NASA/ESA Hubble Space Telescope, shows the star HD 184738, also known as Campbell’s hydrogen star. It is surrounded by plumes of reddish gas — the fiery red and orange hues are caused by glowing gases, including hydrogen and nitrogen.HD 184738 is at the centre of a small planetary nebula. The star itself is known as a [WC] star, a rare class resembling their much more massive counterparts — Wolf-Rayet stars. These stars are named after two French astronomers, Charles Wolf and Georges Rayet, who first identified them in the mid-nineteenth century. Wolf-Rayet stars are hot stars, perhaps 20 times more massive than the Sun, that are rapidly blowing away material and losing mass. [WC] stars are rather different: they are low-mass Sun-like stars at the end of their lives. While these stars have recently ejected much of their original mass, the hot stellar core is still losing mass at a high rate, creating a hot wind. It is these winds that cause them to resemble Wolf-Rayet stars.However, astronomers can look more closely at the composition of these winds to tell the stars apart; [WC] stars are identified by the carbon and oxygen in their winds. Some true Wolf-Rayet stars are rich in nitrogen instead, but this is very rare among their low-mass counterparts. HD 184738 is also very bright in the infrared part of the spectrum, and is surrounded by dust very similar to the material that the Earth formed from. The origin of this dust is uncertain.A version of this image was entered into the Hubble’s Hidden Treasures image processing competition by contestant Jean-Christophe Lambry. This caption was revised on 18/09/2013 to more accurately describe this image.
簡稱	A smouldering star
使用條款	Creative Commons Attribution 4.0 International License
資料產生的日期時間	2013年9月16日 (一) 10:00
關鍵字	Campbell's star HD 184738
聯絡資訊	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei München, , D-85748 Germany
IIM 版本	4

File:A giant, smouldering star.jpg

摘要

授權條款

說明

在此檔案描寫的項目

描繪內容

HD 184738 ^英文

著作權狀態

有著作權

授權條款

創用CC姓名標示4.0國際 ^{繁體中文 (已轉換拼寫)}

成立或建立時間

16 9 2013

多媒體型式

image/jpeg

核對和

f07eea03bf3402e2556250ff4d564b1387f708ff

資料大小

87,689 位元組

高度

501 像素

寬度

501 像素

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

File:A giant, smouldering star.jpg

摘要

授權條款

說明

在此檔案描寫的項目

HD 184738 英文

創用CC姓名標示4.0國際 繁體中文 (已轉換拼寫)

16 9 2013

image/jpeg

f07eea03bf3402e2556250ff4d564b1387f708ff

87,689 位元組

501 像素

501 像素

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

HD 184738 ^英文

創用CC姓名標示4.0國際 ^{繁體中文 (已轉換拼寫)}