NASAs Fermi Gamma-ray Space Telescope has detected a mysterious Galactic Center glow that may be linked to dark matter emissions, challenging our understanding of the Milky Way and the Universe.
- Since its launch in 2008, NASAs Fermi Gamma-ray Space Telescope has observed a persistent gamma ray glow at the Galactic Center, intriguing scientists about its origins.
- Some astronomers hypothesize that the gamma ray emissions are produced by pulsars, the remnants of exploded stars, while others suggest a potential link to dark matter.
- Published findings in Physical Review Letters discuss how the glow could indicate new physics related to dark matter, reshaping our understanding of the galaxy and its composition.
Why It Matters
Understanding the origins of the gamma ray emissions could unlock new insights into dark matter and the structure of the Milky Way, fundamentally altering our comprehension of cosmic phenomena and the Universe.