II* : @ I R ( 1 2 ; = b! A R' s ' I @ `- i `m The supernova remnant1E0102.2-7219 sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy located about 200,000 light-years from Earth. A supernova remnant is made up of the messy bits and pieces of a massive star that exploded, or went supernova. The red bubble is a dust envelope around the supernova remnant E0102, which is being heated by the shock wave created in the explosion of the remnant's massive progenitor star some 1,000 years ago. Most of the blue stars are in the Small Magellanic Cloud, though some are in our own galaxy.
This close-up of E0102 is a composite of the infrared observations by Spitzer (red), an optical image (0.5 microns) captured by NASA's Hubble Space Telescope (green), and X-ray measurements by NASA's Chandra X-ray Observatory (blue). The X-ray ring is generated when the reverse shock slams into stellar material that was expelled during the explosion. m y n , :i D w XK h ` & r ] O} G m F Q4 TD - ' - ' Adobe Photoshop CS3 Macintosh 2009:02:26 10:43:07 Spitzer Space Telescope
Pasadena
USA
1200 E. California Blvd.
91125
CA
http://www.spitzer.caltech.edu
Distance taken from Fast Facts.
2000000
-
Chandra
Hubble
Spitzer
sig06-016b
Good
ACIS
WFPC2
MIPS
2012-10-11
1.1
Spitzer Science Center
spitzer
http://www.spitzer.caltech.edu/images/2207-sig06-016b-Supernova-Remnant-1E0102-2-7219
sig06-016b.tif
http://www.spitzer.caltech.edu/uploaded_files/images/0001/5031/sig06-016b.tif
ICRS
TAN
J2000
Full
1191.0
1191.0
596.5
596.5
16.0096298
-72.0307128
0.2
1.65089e-05
1.65089e-05
X-ray
Optical
Infrared
-
V-band
Mid-IR
0.8267
550
24000
Blue
Green
Red
C.4.1.4.
Observation
Spitzer Space Telescope
The supernova remnant1E0102.2-7219 sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy located about 200,000 light-years from Earth. A supernova remnant is made up of the messy bits and pieces of a massive star that exploded, or went supernova. The red bubble is a dust envelope around the supernova remnant E0102, which is being heated by the shock wave created in the explosion of the remnant's massive progenitor star some 1,000 years ago.
This close-up of E0102 is a composite of the infrared observations by Spitzer (red), an optical image (0.5 microns) captured by NASA's Hubble Space Telescope (green), and X-ray measurements by NASA's Chandra X-ray Observatory (blue). The X-ray ring is generated when the reverse shock slams into stellar material that was expelled during the explosion.
E0102
E0102.2-7219
N76
Supernova Remnant 1E0102.2-7219
NASA
2006-06-06
The supernova remnant 1E0102.2-7219, revealed by NASA's Spitzer Space Telescope, Hubble Space Telescope and Chandra X-ray Observatory, sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy located about 200,000 light-years from Earth.
Spitzer Space Telescope
http://www.spitzer.caltech.edu/info/18-Image-Use-Policy
http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml Z %G xThe supernova remnant1E0102.2-7219 sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy located about 200,000 light-years from Earth. A supernova remnant is made up of the messy bits and pieces of a massive star that exploded, or went supernova. The red bubble is a dust envelope around the supernova remnant E0102, which is being heated by the shock wave created in the explosion of the remnant's massive progenitor star some 1,000 years ago. Most of the blue stars are in the Small Magellanic Cloud, though some are in our own galaxy.
This close-up of E0102 is a composite of the infrared observations by Spitzer (red), an optical image (0.5 microns) captured by NASA's Hubble Space Telescope (green), and X-ray measurements by NASA's Chandra X-ray Observatory (blue). The X-ray ring is generated when the reverse shock slams into stellar material that was expelled during the explosion.i The supernova remnant 1E0102.2-7219, revealed by NASA's Spitzer Space Telescope, Hubble Space Telescope and Chandra X-ray Observatory, sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our MiP Spitzer Space Telescopen NASAs Spitzer Space Telescope Supernova Remnant 1E0102.2-72197 20060606 E0102 E0102.2-7219 N76t @http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml 8BIM Z %G xThe supernova remnant1E0102.2-7219 sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our Milky Way galaxy located about 200,000 light-years from Earth. A supernova remnant is made up of the messy bits and pieces of a massive star that exploded, or went supernova. The red bubble is a dust envelope around the supernova remnant E0102, which is being heated by the shock wave created in the explosion of the remnant's massive progenitor star some 1,000 years ago. Most of the blue stars are in the Small Magellanic Cloud, though some are in our own galaxy.
This close-up of E0102 is a composite of the infrared observations by Spitzer (red), an optical image (0.5 microns) captured by NASA's Hubble Space Telescope (green), and X-ray measurements by NASA's Chandra X-ray Observatory (blue). The X-ray ring is generated when the reverse shock slams into stellar material that was expelled during the explosion.i The supernova remnant 1E0102.2-7219, revealed by NASA's Spitzer Space Telescope, Hubble Space Telescope and Chandra X-ray Observatory, sits next to the nebula N76 in a bright, star-forming region of the Small Magellanic Cloud, a satellite galaxy to our MiP Spitzer Space Telescopen NASAs Spitzer Space Telescope Supernova Remnant 1E0102.2-72197 20060606 E0102 E0102.2-7219 N76t @http://www.spitzer.caltech.edu/Media/mediaimages/copyright.shtml8BIM% XMdc~cq8BIM 1
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