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File:M87 jet.jpg

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原始檔案 (1,222 × 1,276 像素,檔案大小:1.71 MB,MIME 類型:image/jpeg


摘要

描述
English: The jet emerging from the galactic core of M87 (NGC 4486). The jet extends to about 20 arc seconds (absolute length ca. 5 kly).

Composite image of Hubble Telescope observations. The galaxy is too distant for the Hubble Telescope to resolve individual stars; the bright dots in the image are star clusters, assumed to contain some hundreds of thousands of stars each.

Original caption:

"Black Hole-Powered Jet of Electrons and Sub-Atomic Particles Streams From Center of Galaxy M87"
The data used in this image was collected with Hubble's Wide Field Planetary Camera 2 in 1998 by J.A. Biretta, W.B. Sparks, F.D. Macchetto, and E.S. Perlman (STScI). This composite image was compiled by the Hubble Heritage team based on these exposures of ultraviolet, blue, green, and infrared light.
Čeština: Výtrysk plazmatu z jádra galaxie M87, který vychází z okolí černé díry
العربية: تدفق مادي ناتج عن ثقب أسود ينبثق من المنطقة المركزية لمجرة مسييه 87.
日期
來源 HubbleSite: gallery, release.
作者 NASA and The Hubble Heritage Team (STScI/AURA)

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根據最有價值圖像標準,這張圖像被評定为在Messier 87範疇內最有價值的共享資源圖像。你可以在Commons:Valued image candidates/M87 jet.jpg参看它的提名。

授權條款

Public domain
This file is in the public domain because it was created by NASA and ESA. NASA Hubble material (and ESA Hubble material prior to 2009) is copyright-free and may be freely used as in the public domain without fee, on the condition that only NASA, STScI, and/or ESA is credited as the source of the material. This license does not apply if ESA material created after 2008 or source material from other organizations is in use.

The material was created for NASA by Space Telescope Science Institute under Contract NAS5-26555, or for ESA by the Hubble European Space Agency Information Centre. Copyright statement at hubblesite.org or 2008 copyright statement at spacetelescope.org.

For material created by the European Space Agency on the spacetelescope.org site since 2009, use the {{ESA-Hubble}} tag.

說明

添加單行說明來描述出檔案所代表的內容
The AGN at the center of Messier 87 ejecting superheated matter (in the form of plasma) from one of its poles. Most AGN & Quasars also spew out plasma, although most spew out of both their poles.

在此檔案描寫的項目

描繪內容

相對論 繁體中文 (已轉換拼寫)

共享資源質素評價 繁體中文 (已轉換拼寫)

維基共享資源最有價值圖像 中文 (已轉換拼寫)

始於:​25 7 2010

多媒體型式 繁體中文 (已轉換拼寫)

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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2007年3月14日 (三) 10:51於 2007年3月14日 (三) 10:51 版本的縮圖1,222 × 1,276(1.71 MB)Tevatron~commonswiki{{Information |Description= Streaming out from the center of the galaxy M87 like a cosmic searchlight is one of nature's most amazing phenomena, a black-hole-powered jet of electrons and other sub-atomic particles traveling at nearly the speed of light. I
2005年7月28日 (四) 13:47於 2005年7月28日 (四) 13:47 版本的縮圖1,222 × 1,276(1.71 MB)Dbenbenn1222 x 1276 version, from http://imgsrc.hubblesite.org/hu/db/2000/20/images/a/formats/full_jpg.jpg
2005年4月9日 (六) 20:52於 2005年4月9日 (六) 20:52 版本的縮圖611 × 638(42 KB)Bebenko~commonswikifrom http://hubblesite.org/newscenter/newsdesk/archive/releases/2000/20/ {{PD-USGov-NASA}} M87 jet.jpg

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