Plik:GLIMPSE-MIPSGAL Milky Way 11.jpg
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OpisGLIMPSE-MIPSGAL Milky Way 11.jpg |
English: This is one segment of an infrared portrait of dust and stars radiating in the inner Milky Way. More than 800,000 frames from NASA's Spitzer Space Telescope were stitched together to create the full image, capturing more than 50 percent of our entire galaxy.
As inhabitants of a flat galactic disk, Earth and its solar system have an edge-on view of their host galaxy, like looking at a glass dish from its edge. From our perspective, most of the galaxy is condensed into a blurry narrow band of light that stretches completely around the sky, also known as the galactic plane. This segment extends through the constellations Scorpius, Ara, and Norma. The flat band of green running through this region is mostly dust in the distant disk of the Milky Way galaxy. In visible light the foreground dust renders this area nearly featureless and dark with only a scattering of nearby stars. The swaths of green represent organic molecules, called polycyclic aromatic hydrocarbons, which are illuminated by light from nearby star formation, while the thermal emission, or heat, from warm dust is rendered in red. Star-forming regions appear as swirls of red and yellow, where the warm dust overlaps with the glowing organic molecules. The blue specks sprinkled throughout the photograph are Milky Way stars. This survey segment spans galactic longitudes of 335.2 to 343.5 degrees and is centered at a galactic latitude of 0 degrees. It covers about two vertical degrees of the galactic plane. This is a three-color composite that shows infrared observations from two Spitzer instruments. Blue represents 3.6-micron light and green shows light of 8 microns, both captured by Spitzer's infrared array camera. Red is 24-micron light detected by Spitzer's multiband imaging photometer. This combines observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and MIPSGAL projects. |
Data | |
Źródło | http://www.spitzer.caltech.edu/images/3366-ssc2008-11a11-GLIMPSE-MIPSGAL-Milky-Way-11 |
Autor | NASA/JPL-Caltech/Univ. of Wisconsin |
Image use policy: http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
Licencja
Public domainPublic domainfalsefalse |
Ten plik jest w domenie publicznej ponieważ został stworzony przez NASA. Polityka praw autorskich NASA stwierdza, że „materiały NASA nie są chronione prawami autorskimi, chyba że zapisano inaczej”. (NASA copyright policy lub JPL Image Use Policy). | ||
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przedstawia
3 cze 2008
image/jpeg
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Data i czas | Miniatura | Wymiary | Użytkownik | Opis | |
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aktualny | 18:53, 14 cze 2011 | 6000 × 3277 (2,19 MB) | Spitzersteph |
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Tytuł lub opis obrazu | This is one segment of an infrared portrait of dust and stars radiating in the inner Milky Way. More than 800,000 frames from NASA's Spitzer Space Telescope were stitched together to create the full image, capturing more than 50 percent of our entire galaxy.
As inhabitants of a flat galactic disk, Earth and its solar system have an edge-on view of their host galaxy, like looking at a glass dish from its edge. From our perspective, most of the galaxy is condensed into a blurry narrow band of light that stretches completely around the sky, also known as the galactic plane. This segment extends through the constellations Scorpius, Ara, and Norma. The flat band of green running through this region is mostly dust in the distant disk of the Milky Way galaxy. In visible light the foreground dust renders this area nearly featureless and dark with only a scattering of nearby stars. The swaths of green represent organic molecules, called polycyclic aromatic hydrocarbons, which are illuminated by light from nearby star formation, while the thermal emission, or heat, from warm dust is rendered in red. Star-forming regions appear as swirls of red and yellow, where the warm dust overlaps with the glowing organic molecules. The blue specks sprinkled throughout the photograph are Milky Way stars. This survey segment spans galactic longitudes of 335.2 to 343.5 degrees and is centered at a galactic latitude of 0 degrees. It covers about two vertical degrees of the galactic plane. This is a three-color composite that shows infrared observations from two Spitzer instruments. Blue represents 3.6-micron light and green shows light of 8 microns, both captured by Spitzer's infrared array camera. Red is 24-micron light detected by Spitzer's multiband imaging photometer. This combines observations from the Galactic Legacy Infrared Mid-Plane Survey Extraordinaire (GLIMPSE) and MIPSGAL projects. |
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Właściciel praw autorskich | http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml |
Szerokość | 24 752 px |
Wysokość | 13 520 px |
Metoda kompresji | LZW |
Interpretacja fotometryczna | RGB |
Orientacja obrazu | normalna |
Próbek na piksel | 3 |
Rozdzielczość w poziomie | 72 punktów na cal |
Rozdzielczość w pionie | 72 punktów na cal |
Rozkład danych | format masywny |
Użyte oprogramowanie | Adobe Photoshop CS3 Macintosh |
Data i czas modyfikacji pliku | 10:45, 13 wrz 2010 |
Przestrzeń kolorów | Nie skalibrowano |