File:G19 xray.tif
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Summary
G1.9+0.3 is the remains of the most recent supernova, in Earth's time frame, known to have occurred in the Milky Way. If gas and dust had not heavily obscured it, the explosion would have been visible from Earth just over a century ago. A new long Chandra observation - equivalent to over 11 days of time - reveals new details about the explosion.
Fast Facts for G1.9+0.3:
Credit X-ray (NASA/CXC/NCSU/K.Borkowski et al.) Release Date June 26, 2013 Scale Image is 8 arcmin across (About 60 light years) Category Supernovas & Supernova Remnants Coordinates (J2000) RA 17h 48m 45s - Dec -27° 10' 00" Constellation Sagittarius Observation Date 15 pointings between Feb 2007 and Jul 2011 Observation Time 362 hours (15 days 2 hours) Obs. ID 6708, 8521, 10111, 10112, 10928, 10930, 12689-95, 13407, 13509 Instrument ACIS References Borkowski, K, et al, 2013, ApJ Letters (Submitted); arXiv:1305.7399 Color Code X-ray (Red, Green, Blue)
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File history
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Date/Time | Thumbnail | Dimensions | User | Comment | |
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current | 02:52, 15 January 2017 | 1,500 × 1,280 (804 KB) | 127.0.0.1 (talk) | G1.9+0.3 is the remains of the most recent supernova, in Earth's time frame, known to have occurred in the Milky Way. If gas and dust had not heavily obscured it, the explosion would have been visible from Earth just over a century ago. A new long Chandra observation - equivalent to over 11 days of time - reveals new details about the explosion. <p>Fast Facts for G1.9+0.3: </p> <pre>Credit X-ray (NASA/CXC/NCSU/K.Borkowski et al.) Release Date June 26, 2013 Scale Image is 8 arcmin across (About 60 light years) Category Supernovas & Supernova Remnants Coordinates (J2000) RA 17h 48m 45s - Dec -27° 10' 00" Constellation Sagittarius Observation Date 15 pointings between Feb 2007 and Jul 2011 Observation Time 362 hours (15 days 2 hours) Obs. ID 6708, 8521, 10111, 10112, 10928, 10930, 12689-95, 13407, 13509 Instrument ACIS References Borkowski, K, et al, 2013, ApJ Letters (Submitted); arXiv:1305.7399 Color Code X-ray (Red, Green, Blue) </pre> . |
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