On Earth, radioactive decay of unstable isotopes in the crust contributes to the natural background radiation that surrounds us constantly. Protection relies on minimizing exposure time, maximizing distance from the source, and using dense shielding materials like lead or thick concrete walls.
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Nuclear explosions, such as those from supernovae and hypernovae, generate vast bursts of this energy as massive stars collapse. This treatment, known as radiotherapy, damages the DNA of cancer cells, preventing them from dividing and growing.
Additionally, matter accelerating around supermassive black holes in active galactic nuclei creates continuous emissions. Key Properties at a Glance Property Description Wavelength Less than 0.
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Space-based observatories like the Fermi Gamma-ray Space Telescope map the sky in high energy light, revealing neutron stars, black holes, and the afterglow of the Big Bang. This research helps test the fundamental laws of physics under conditions that cannot be replicated on Earth.
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