Evidence emerges that intense stellar explosions send high-energy protons hurtling through the galaxy
Remnants of two supernovas have provided the best proof yet that
supernova shock waves churn out the high-energy protons that whizz
through the galaxy.
Many of these speedy protons, better known as cosmic rays, have
more energy than those in any manmade particle accelerator. Astronomers
spent four years probing W44, the remains of a supernova located about
10,000 light-years away in the constellation Aquila, and another remnant
called IC 433, located roughly 5,000 light-years away in the
constellation Gemini, with NASA’s Fermi Gamma-ray Space Telescope. The
scope picked up a steady stream of gamma radiation at energies that
could only have come from a nuclear reaction involving cosmic rays
slamming into slower-moving interstellar material, researchers report in
the Feb. 15 Science.
Scientists have long suspected that protons become cosmic rays
when they get energy boosts from interacting with rapidly expanding
supernova shock waves. But in the absence of strong observational
evidence, some skeptics had proposed other mechanisms. “This measurement
puts those theories to rest,” says Stanford University astrophysicist
and study author Stefan Funk. “This is definitive proof that protons are
accelerated in supernova remnants.”
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