LHAASO J1912+1014u Confirmed as 1 PeV Proton Accelerator, Outpacing the LHC
Updated
Updated · Gizmodo · Aug 5
LHAASO J1912+1014u Confirmed as 1 PeV Proton Accelerator, Outpacing the LHC
2 articles · Updated · Gizmodo · Aug 5
Summary
Scientists confirmed LHAASO J1912+1014u is a Milky Way PeVatron, showing it accelerates protons beyond 1 quadrillion electron volts rather than merely emitting ambiguous gamma rays.
Three observatories—Fermi-LAT, FUGIN and Chandra—let researchers build a multi-wavelength model that ruled out electrons as the source of the gamma-ray signal.
First spotted in 2024 near Altair and initially tagged as a supernova remnant, the object still has no identified engine even though its proton acceleration is now established.
One PeV is thousands of times more energetic than the Large Hadron Collider’s maximum collision energy, making the source a key clue to the origin of the galaxy’s highest-energy cosmic rays.
The result, published in The Astrophysical Journal, also suggests dozens of similar natural accelerators may be scattered across the Milky Way and gives astronomers a clearer way to find them.
In August 2026, scientists confirmed LHAASO J1912+1014u as a Galactic proton PeVatron by combining data from Fermi-LAT, FUGIN, and Chandra. Their multiwavelength model ruled out electrons and showed that protons are accelerated by shock waves from supernova remnants. These protons gain energy through repeated crossings of the shock front, eventually reaching ultra-high energies and escaping as cosmic rays. Because cosmic rays are charged, their paths are scrambled by interstellar magnetic fields, making it hard to trace them back to their source. This breakthrough solved a century-old mystery about the origin of cosmic rays and validated key theories in astrophysics.