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tóng-àn:A Swarm of Ancient Stars - GPN-2000-000930.jpg

Choân kái-sek-tō͘ ‎（1,777 × 1,864 siōng-sò͘ , tóng-àn chiàm-liōng: 4.03 MB, MIME luī-hêng: image/jpeg）

Soat-bêng
English: This stellar swarm is M80 (NGC 6093), one of the densest of the 147 known globular star clusters in the Milky Way galaxy. Located about 28,000 light-years from Earth, M80 contains hundreds of thousands of stars, all held together by their mutual gravitational attraction. Globular clusters are particularly useful for studying stellar evolution, since all of the stars in the cluster have the same age (about 12 billion years), but cover a range of stellar masses. Every star visible in this image is either more highly evolved than, or in a few rare cases more massive than, our own Sun. Especially obvious are the bright red giants, which are stars similar to the Sun in mass that are nearing the ends of their lives.
Ji̍t-kî
Chhut-chhù Great Images in NASA Description
Chok-chiá NASA, The Hubble Heritage Team, STScI, AURA
授權允准
(Bô siŏh-huòi sāi ciā ùng-giông)
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.
本圖像或影音收錄於美國國家航空暨太空總署 （NASA）太空望遠鏡研究所（Space Telescope Science Institute），其照片編號為： GPN-2000-000930 以及Alternate ID: PR99-26

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說明

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Star Swarms

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描繪內容 繁體中文

多媒體型式 繁體中文

image/jpeg

校驗和 繁體中文

71a8b3eb2ddd1ab70f006560b8467fd3edcc4f69

斷定方法 繁體中文: SHA-1 中文 (已轉換拼寫)

資料大小 繁體中文

4,224,281 Byte

高度 繁體中文

1,864 ōe-sò͘

寬度 繁體中文

1,777 ōe-sò͘

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Ji̍t-kî/Sî-kanSáuk-liŏk-dùChióh-cháungIōng-chiáChù-kái
hiān-chāi2010-nî 3-goe̍h 4-ji̍t (pài-sì) 14:082010-nî 3-goe̍h 4-ji̍t (pài-sì) 14:08 bēng-buōng gì sáuk-liŏk-dù1,777 × 1,864（4.03 MB）TryphonFrom original source http://hubblesite.org/newscenter/archive/releases/1999/26/image/a/ (http://imgsrc.hubblesite.org/hu/db/images/hs-1999-26-a-full_jpg.jpg).
2009-nî 4-goe̍h 9-ji̍t (pài-sì) 00:542009-nî 4-goe̍h 9-ji̍t (pài-sì) 00:54 bēng-buōng gì sáuk-liŏk-dù1,777 × 1,864（3.98 MB）BotMultichillT{{Information |Description={{en|1=This stellar swarm is M80 (NGC 6093), one of the densest of the 147 known globular star clusters in the Milky Way galaxy. Located about 28,000 light-years from Earth, M80 contains hundreds of thousands of stars, all held

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