News / Science News |
Trigger for Milky Way’s Youngest Supernova Identified
NASA | MARCH 31, 2016
Astronomers had previously identified G1.9+0.3 as the remnant of the most recent supernova in our Galaxy. It is estimated to have occurred about 110 years ago in a dusty region of the Galaxy that blocked visible light from reaching Earth.
G1.9+0.3 belongs to the Type Ia category, an important class of supernovas exhibiting reliable patterns in their brightness that make them valuable tools for measuring the rate at which the universe is expanding.
Astronomers use Type Ia supernovas as distance markers across the Universe, which helped us discover that its expansion was accelerating. If there are any differences in how these supernovas explode and the amount of light they produce, that could have an impact on our understanding of this expansion.
Most scientists agree that Type Ia supernovas occur when white dwarfs, the dense remnants of Sun-like stars that have run out of fuel, explode. However, there has been a debate over what triggers these white dwarf explosions. Two primary ideas are the accumulation of material onto a white dwarf from a companion star or the violent merger of two white dwarfs.
The new research with archival Chandra and VLA data examines how the expanding supernova remnant G1.0+0.3 interacts with the gas and dust surrounding the explosion. The resulting radio and X-ray emission provide clues as to the cause of the explosion. In particular, an increase in X-ray and radio brightness of the supernova remnant with time, is expected only if a white dwarf merger took place.
The team also derived a new estimate for the age of the supernova remnant of about 110 years, younger than previous estimates of about 150 years.