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| NASA/JPL-Caltech/Univ. of Wisconsin |
Spitzer Finds Clarity in the Inner Milky Way
More than 800,000 frames from NASA's Spitzer Space Telescope were stitched together to create this infrared portrait of dust and stars radiating in the inner Milky Way.
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.
In this mosaic the galactic plane is broken up into five components: the far-left side of the plane (top image); the area just left of the galactic center (second to top); galactic center (middle); the area to the right of galactic center (second to bottom); and the far-right side of the plane (bottom). From Earth, the top two panels are visible to the northern hemisphere, and the bottom two images to the southern hemisphere. Together, these panels represent more than 50 percent of our entire Milky Way galaxy.
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. The bluish-white haze that hovers heavily in the middle panel is starlight from the older stellar population towards the center of the galaxy.
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.
The Galactic Legacy Infrared Mid-Plane Survey Extraordinaire team (GLIMPSE) used the telescope's infrared array camera to see light from newborn stars, old stars and polycyclic aromatic hydrocarbons. A second group, the Multiband Imaging Photometer for Spitzer Galactic Plane Survey team (MIPSGAL), imaged dust in the inner galaxy with Spitzer's multiband imaging photometer.
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| About the Object |
Object Name:
Milky Way, Galactic Plane
Object Type:
Galaxy
Position (J2000):
RA:
17h 45m 40.00s
Dec:
-29d 0m 28.00s
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| About the Data |
Image Credit:
NASA/JPL-Caltech/(Univ. of Wisconsin)
Instrument:
IRAC, MIPS
Release Date:
June 3, 2008
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INDIVIDUAL IMAGES
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Mosaic Tile 1 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 2 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 3 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 4 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 5 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 6 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 7 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 8 of 16 (Left to Right)
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Credit: NASA/JPL-Caltech/Univ. of Wisconsin
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Mosaic Tile 9 of 16 (Left to Right)
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Mosaic Tile 10 of 16 (Left to Right)
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Mosaic Tile 11 of 16 (Left to Right)
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Mosaic Tile 12 of 16 (Left to Right)
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Mosaic Tile 13 of 16 (Left to Right)
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Mosaic Tile 14 of 16 (Left to Right)
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Mosaic Tile 15 of 16 (Left to Right)
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Mosaic Tile 16 of 16 (Left to Right)
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