File:A spiral home to exploding stars.jpg

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描述A spiral home to exploding stars.jpg	English: In this new Hubble image, we can see an almost face-on view of the galaxy NGC 1084. At first glance, this galaxy is pretty unoriginal. Like the majority of galaxies that we observe it is a spiral galaxy, and, as with about half of all spirals, it has no bar running through its loosely wound arms. However, although it may seem unremarkable on paper, NGC 1084 is actually a near-perfect example of this type of galaxy — and Hubble has a near-perfect view of it. NGC 1084 has hosted several violent events known as supernovae — explosions that occur when massive stars, many times more massive than the Sun, approach their twilight years. As the fusion processes in their cores run out of fuel and come to an end, these stellar giants collapse, blowing off their outer layers in a violent explosion. Supernovae can often briefly outshine an entire galaxy, before then fading away over several weeks or months. Although directly observing one of these explosions is hard to do, in galaxies like NGC 1084 astronomers can find and study the remnants left behind. Astronomers have noted five supernova explosions within NGC 1084 over the past half century. These remnants are named after the year in which they took place — 1963P, 1996an, 1998dl, 2009H, and 2012ec. The most recent explosion, 2012ec, was detected at the end of NGC 1084’s top right arm in August 2012. It is not visible here as these images were taken in 2001, some eleven years before this supernova exploded. Astronomers at Queen's University Belfast have managed to use these "before" images to directly identify the star that exploded. It appears to be a red supergiant some 10 to 20 times more massive than the Sun, and quite similar to the well-known star Betelguese in Orion. A version of this image was entered into the Hubble's Hidden Treasures image processing competition by Flickr user Brian Campbell (Sinickel).
日期	2014年3月31日, 10:00:00
來源	http://www.spacetelescope.org/images/potw1413a/
作者	NASA, ESA, and S. Smartt (Queen's University Belfast) Acknowledgement: Brian Campbell

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	日期/時間	縮⁠圖	尺寸	使用者	備⁠註
目前	2014年3月31日 (一) 23:09		2,134 × 1,953（2.29 MB）	Jmencisom	User created page with UploadWizard

檔案用途

下列頁面有用到此檔案：

螺旋星系

全域檔案使用狀況

以下其他 wiki 使用了這個檔案：

ar.wikipedia.org 的使用狀況
- NGC 1084
ca.wikipedia.org 的使用狀況
- Galàxia espiral
de.wikipedia.org 的使用狀況
- NGC 1084
el.wikipedia.org 的使用狀況
- NGC 1084
en.wikipedia.org 的使用狀況
en.wikiquote.org 的使用狀況
- Milky Way
eu.wikipedia.org 的使用狀況
- Galaxia
fa.wikipedia.org 的使用狀況
- ان‌جی‌سی ۱۰۸۴
fr.wikipedia.org 的使用狀況
- NGC 1084
it.wikipedia.org 的使用狀況
ko.wikipedia.org 的使用狀況
- 나선은하
lb.wikipedia.org 的使用狀況
- NGC 1084
mk.wikipedia.org 的使用狀況
- Спирална галаксија
pl.wikipedia.org 的使用狀況
- NGC 1084

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來源	ESA/Hubble
製作/提供者	NASA, ESA, and S. Smartt (Queen's University Belfast)Acknowledgement: Brian Campbell
影像標題	In this new Hubble image, we can see an almost face-on view of the galaxy NGC 1084. At first glance, this galaxy is pretty unoriginal. Like the majority of galaxies that we observe it is a spiral galaxy, and, as with about half of all spirals, it has no bar running through its loosely wound arms. However, although it may seem unremarkable on paper, NGC 1084 is actually a near-perfect example of this type of galaxy— and Hubble has a near-perfect view of it. NGC 1084 has hosted several violent events known as supernovae — explosions that occur when massive stars, many times more massive than the Sun, approach their twilight years. As the fusion processes in their cores run out of fuel and come to an end, these stellar giants collapse, blowing off their outer layers in a violent explosion. Supernovae can often briefly outshine an entire galaxy, before then fading away over several weeks or months. Although directly observing one of these explosions is hard to do, in galaxies like NGC 1084 astronomerscan find and study the remnants left behind. Astronomers have noted five supernova explosions within NGC 1084 over the past half century. These remnants are named after the year in which they took place — 1963P, 1996an, 1998dl, 2009H, and 2012ec. The most recent explosion, 2012ec, was detected atthe end of NGC 1084’s top right arm in August 2012. It is not visible here as these images were taken in 2001, some eleven years before this supernova exploded. Astronomers at Queen's University Belfast have managed to use these "before" images to directly identify the star that exploded. It appears to be a red supergiant some 10 to 20 times more massive than the Sun, and quite similar to the well-known star Betelguese in Orion. A version of this image was entered into the Hubble's Hidden Treasures image processing competition by Flickr user Brian Campbell (Sinickel).
簡稱	A spiral home to exploding stars
使用條款	Creative Commons Attribution 3.0 Unported license
資料產生的日期時間	2014年3月31日 (一) 10:00
使用軟體	Adobe Photoshop CS6 (Windows)
原始文件唯一識別碼	xmp.did:86F5805E1C25E311A5A4C3FD8C3E8B93
關鍵字	NGC 1084
聯絡資訊	http://www.spacetelescope.org/ Karl-Schwarzschild-Strasse 2 Garching bei M√ºnchen, , D-85748 Germany

File:A spiral home to exploding stars.jpg

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創用CC姓名標示4.0國際 ^{繁體中文 (已轉換拼寫)}

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File:A spiral home to exploding stars.jpg

摘要

授權條款

說明

在此檔案描寫的項目

沒有維基數據項目的某些值

創用CC姓名標示4.0國際 繁體中文 (已轉換拼寫)

31 3 2014

image/jpeg

d11916feadcc79a48535fb3824943016bb0d3463

2,397,245 位元組

1,953 像素

2,134 像素

檔案歷史

檔案用途

全域檔案使用狀況

詮釋資料

創用CC姓名標示4.0國際 ^{繁體中文 (已轉換拼寫)}