File:Rcw49 spitzer c1.jpg
原始檔案 (1,520 × 1,520 像素,檔案大小:414 KB,MIME 類型:image/jpeg)
摘要
描述Rcw49 spitzer c1.jpg |
English: RCW 49 by the Spitzer Space Telescope.
NASA: Observation • May 27th, 2004 • ssc2004-08a1 ssc2004-08a1 One of the most prolific birthing grounds in our Milky Way galaxy, a nebula called RCW 49, is exposed in superb detail for the first time in this new image from NASA's Spitzer Space Telescope. Located 13,700 light-years away in the southern constellation Centaurus, RCW 49 is a dark and dusty stellar nursery that houses more than 2,200 stars. Because many of the stars in RCW 49 are deeply embedded in plumes of dust, they cannot be seen at visible wavelengths. When viewed with Spitzer's infrared eyes, however, RCW 49 becomes transparent. Like cracking open a quartz rock to discover its jewels inside, the nebula's newborn stars have been dramatically exposed. This image taken by Spitzer's infrared array camera highlights the nebula's older stars (blue stars in center pocket), its gas filaments (green) and dusty tendrils (pink). Speckled throughout the murky clouds are more than 300 never-before-seen newborn stars. Astronomers are interested in further studying these newfound proto-stars because they offer a fresh look at star formation in our own galaxy. This image was taken on Dec. 23, 2003, and is composed of photographs obtained at four wavelengths: 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). |
日期 | |
來源 | Spitzer/Caltech/NASA |
作者 | NASA/JPL-Caltech/E. Churchwell (University of Wisconsin) |
授權條款
Public domainPublic domainfalsefalse |
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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原始上傳日誌
日期/時間 | 尺寸 | 用戶 | 備註 |
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2010-09-01 06:31:34 | 638× 515× | Mohamed Osama AlNagdy | {{Information |Description={{en|1=RCW 49 by the [[Spitzer Space Telescope]].}} |Source=http://apod.nasa.gov/apod/ap040603.html |Author=NASA |Date=2003-12-23 |Permission= |other_versions= }} |
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23 12 2003
多媒體型式 繁體中文 (已轉換拼寫)
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目前 | 2023年1月15日 (日) 16:27 | 1,520 × 1,520(414 KB) | Liandrei | Higher res version (from: https://www.spitzer.caltech.edu/image/ssc2004-08a1-star-formation-in-rcw-49) | |
2016年11月5日 (六) 20:28 | 638 × 515(47 KB) | Zppix | Transferred from en.wikipedia (MTC!) |
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影像標題 | One of the most prolific birthing grounds in our Milky Way galaxy, a nebula called RCW 49, is exposed in superb detail for the first time in this new image from NASA's Spitzer Space Telescope. Located 13,700 light-years away in the southern constellation Centaurus, RCW 49 is a dark and dusty stellar nursery that houses more than 2,200 stars. Because many of the stars in RCW 49 are deeply embedded in plumes of dust, they cannot be seen at visible wavelengths. When viewed with Spitzer's infrared eyes, however, RCW 49 becomes transparent. Like cracking open a quartz rock to discover its jewels inside, the nebula's newborn stars have been dramatically exposed. This image taken by Spitzer's infrared array camera highlights the nebula's older stars (blue stars in center pocket), its gas filaments (green) and dusty tendrils (pink). Speckled throughout the murky clouds are more than 300 never-before-seen newborn stars. Astronomers are interested in further studying these newfound proto-stars because they offer a fresh look at star formation in our own galaxy. This image was taken on Dec. 23, 2003, and is composed of photographs obtained at four wavelengths: 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). |
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標題 | One of the most prolific birthing grounds in our Milky Way galaxy, a nebula called RCW 49, is exposed in superb detail for the first time in this image from NASA's Spitzer Space Telescope. Located 13,700 light-years away in the southern constellation Cent |
作者 | Spitzer Space Telescope |
製作/提供者 | NASA/JPL-Caltech/E. Churchwell ( |
來源 | Spitzer Space Telescope |
簡稱 | Star Formation in RCW 49 |
資料產生的日期時間 | 2004年5月27日 (星期四) |
版權所有人 | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
JPEG 檔案備註 | One of the most prolific birthing grounds in our Milky Way galaxy, a nebula called RCW 49, is exposed in superb detail for the first time in this new image from NASA's Spitzer Space Telescope. Located 13,700 light-years away in the southern constellation Centaurus, RCW 49 is a dark and dusty stellar nursery that houses more than 2,200 stars.
Because many of the stars in RCW 49 are deeply embedded in plumes of dust, they cannot be seen at visible wavelengths. When viewed with Spitzer's infrared eyes, however, RCW 49 becomes transparent. Like cracking open a quartz rock to discover its jewels inside, the nebula's newborn stars have been dramatically exposed. This image taken by Spitzer's infrared array camera highlights the nebula's older stars (blue stars in center pocket), its gas filaments (green) and dusty tendrils (pink). Speckled throughout the murky clouds are more than 300 never-before-seen newborn stars. Astronomers are interested in further studying these newfound proto-stars because they offer a fresh look at star formation in our own galaxy. This image was taken on Dec. 23, 2003, and is composed of photographs obtained at four wavelengths: 3.6 microns (blue), 4.5 microns (green), 5.8 microns (orange) and 8 microns (red). |
IIM 版本 | 2 |
關鍵字 |
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聯絡資訊 |
http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA |