Податотека:Rcw49 spitzer c1.jpg
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Изворна податотека (1.520 × 1.520 пиксели, големина: 414 КБ, MIME-тип: image/jpeg)
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Опис
ОписRcw49 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). |
Датум | |
Извор | Spitzer/Caltech/NASA |
Автор | NASA/JPL-Caltech/E. Churchwell (University of Wisconsin) |
Лиценцирање
Public domainPublic domainfalsefalse |
Оваа податотека е во јавна сопственост бидејќи нејзин создавач е НАСА. Правилата за авторски права на НАСА велат: „Материјалот на НАСА не е заштитен со авторски права освен ако не е поинаку нагласено“. (Правилата за авторски дела на НАСА или правила за користење на слики од Лабораторијата за реактивен погон (JPL)). | ||
Предупредувања:
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Изворна евиденција за подигањето
Датум/време | Димензии | Корисник | Коментар |
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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= }} |
Предмети прикажани на податотекава
прикажува
23 декември 2003
image/jpeg
Историја на податотеката
Стиснете на датум/време за да ја видите податотеката како изгледала тогаш.
Датум/време | Минијатура | Димензии | Корисник | Коментар | |
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тековна | 18:27, 15 јануари 2023 | 1.520 × 1.520 (414 КБ) | Liandrei | Higher res version (from: https://www.spitzer.caltech.edu/image/ssc2004-08a1-star-formation-in-rcw-49) | |
22:28, 5 ноември 2016 | 638 × 515 (47 КБ) | Zppix | Transferred from en.wikipedia (MTC!) |
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Метаподатоци
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Наслов на сликата | 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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Наслов | 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 |
Автор | Spitzer Space Telescope |
Припишување/Објавувач | NASA/JPL-Caltech/E. Churchwell ( |
Извор | Spitzer Space Telescope |
Краток наслов | Star Formation in RCW 49 |
Датум и време на сликање | 27 мај 2004 |
Праводржец | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Забелешка за JPEG-сликата | 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-верзија | 2 |
Клучни зборови |
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Контактни податоци |
http://www.spitzer.caltech.edu 1200 E. California Blvd. Pasadena, CA, 91125 USA |