File:W5 cropped.jpg
![File:W5 cropped.jpg](https://upload.wikimedia.org/wikipedia/commons/thumb/b/b9/W5_cropped.jpg/800px-W5_cropped.jpg?20170513140032)
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描述W5 cropped.jpg |
English: From the source site, courtesy of NASA/JPL-Caltech: Generations of stars can be seen in this new infrared portrait from NASA's Spitzer Space Telescope. In this wispy star-forming region, called W5, the oldest stars can be seen as blue dots in the centers of the two hollow cavities (other blue dots are background and foreground stars not associated with the region). Younger stars line the rims of the cavities, and some can be seen as pink dots at the tips of the elephant-trunk-like pillars. The white knotty areas are where the youngest stars are forming. Red shows heated dust that pervades the region's cavities, while green highlights dense clouds.
W5 spans an area of sky equivalent to four full moons and is about 6,500 light-years away in the constellation Cassiopeia. The Spitzer picture was taken over a period of 24 hours.
Français : Traduction française de la légende originale de la NASA/JPL-Caltech : Image infrarouge du télescope spatial Spitzer représentant la région W5, une zone de formation d'étoiles couvrant la surface de quatre pleines lunes. Plusieurs générations d'histoire peuvent être vues sur cette image. Les étoiles les plus vieilles sont visibles sous la forme de points de lumière bleue au centre des deux cavités vides (Les autres points bleus sont des étoiles plus proches ou plus éloignées que W5). Des étoiles plus jeunes sont sur le bord de ces cavités, et d'autres sont visibles sous la forme de points roses au sommet des piliers. Les étoiles les plus jeunes sont en train de se former dans les zones grumeleuses blanches. Le rouge marque la poussière chaude qui occupe les cavités de cette région, et le vert marque les nuages denses. |
日期 |
20年代 date QS:P,+20-00-00T00:00:00Z/8 eptember 2006, 28 September 2006, 16 February 2007 (IRAC); 23 February 2006 (MIPS) |
來源 | [1] |
作者 | NASA/JPL-Caltech |
授權許可 (重用此檔案) |
Unless otherwise noted, images and video on Spitzer public web sites (public sites ending with a spitzer.caltech.edu address) may be used for any purpose without prior permission ([2]). |
其他版本 | Image:W5.jpg |
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This image was selected as picture of the day on Wikimedia Commons for 29 September 2009. It was captioned as follows: English: Generations of stars can be seen in this new infrared portrait from NASA's Spitzer Space Telescope. Other languages:
Bosanski: Generacije zvijezda mogu biti viđene na ovoj novoj infracrvenoj slici sa Nasinog teleskopa Spitzer Space. Čeština: Na této nové infračervené fotografii ze Spitzerova vesmírného dalekohledu je možno vidět mnoho generací hvězd Dansk: Infrarødt billede fra NASAs Spitzer-rumteleskop af stjernedannelsestågen W5 i stjernebilledet Cassiopeia. W5 ligger omkring 6.500 lysår fra Jorden og dækker et område af himlen, som svarer til fire fuldmåner. Deutsch: Infrarotaufnahme des Spitzer-Weltraumteleskops der Region W5 in der die Entstehung neuer Sterne beobachtet werden kann English: Generations of stars can be seen in this new infrared portrait from NASA's Spitzer Space Telescope. Español: Imagen infrarroja, tomada por el telescopio espacial Spitzer, de la región W5 (Casiopea), una zona de formación de nuevas estrellas. Français : Image infrarouge du télescope spatial Spitzer représentant la région W5, une zone de formation d'étoiles couvrant la surface de quatre pleines lunes. Italiano: Immagine all'infrarosso in falsi colori ripresa dal Telescopio spaziale Spitzer della regione di formazione stellare di Cassiopea W5. Nederlands: infraroodafbeelding van de emissienevel W5 (IC 1871 of "zielnevel") in het H-II-gebied in het sterrenbeeld Cassiopeia gemaakt door de Spitzer Space Telescope van de Nasa. W5 ligt op ongeveer 6.500 lichtjaren van de Aarde verwijderd, omspant een gebied ter grootte van vier volle manen en vormt een stervorminggebied. De foto, die werd gemaakt over een periode van 24 uur, vormt een van de beste bewijzen voor de theorie van de 'getriggerde stervorming'; een bepaalde oorzaak die leidt tot de zwaartekrachtinstorting van een moleculaire wolk. Polski: Pokolenia gwiazd widoczne na zdjęciu w podczerwieni wykonanym przez teleskop Spitzer Space należący do NASA. Português: Imagem em infravermelho da região de formação estelar W5 (Allen), captada pelo telescópio espacial Spitzer, da NASA. Македонски: Генерации на ѕвезди на нова инфрацрвена снимка на вселенскиот телескоп „Спицер“ на НАСА. Русский: Область звездообразования W5 в созвездии Кассиопея. Инфракрасная фотография, сделанная космическим телескопом Спитцер |
Public domainPublic domainfalsefalse |
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本作品由NASA創作,屬於公有領域。根據NASA的版權政策:“NASA的創作除非另有聲明否則不受版權保護。”(參見:Template:PD-USGov/zh,NASA版權政策或JPL圖像使用政策) | ![]() |
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