新的Fermi望远镜数据表明,银河系中心的神秘伽马射线发光可能发出暗物质信号。 A mysterious gamma-ray glow at the Milky Way’s center may signal dark matter, new Fermi Telescope data suggests.

根据最近利用美国航天局的Fermi望远镜数据得出的调查结果,银河系中心的持久性伽马射线发光可能暗示暗物质。 A persistent gamma-ray glow at the Milky Way’s center may hint at dark matter, according to recent findings using data from NASA’s Fermi Telescope. 超过7000光年的信号与暗物质粒子灭绝的预测相匹配,尽管来自毫秒脉冲星的排放仍然是一个可能的解释。 The signal, spanning 7,000 light-years, matches predictions for dark matter particle annihilation, though emissions from millisecond pulsars remain a possible explanation. 新的模拟支持暗物质理论,但两种假设都没有被证实。 New simulations support the dark matter theory, but neither hypothesis is confirmed. 从2026年开始,Cherenkov望远镜阵列即将观测到的观测结果可能有助于区分两者。 Upcoming observations from the Cherenkov Telescope Array, starting in 2026, could help distinguish between them. 虽然暗物质从未被直接观测过,但其引力效应是有据可查的,这一发现为正在进行的了解其性质的努力增添了巨大势头。 While dark matter has never been directly observed, its gravitational effects are well-documented, and this discovery adds significant momentum to ongoing efforts to understand its nature.