这是人类首次捕捉到如此极端的黑洞"进食"现场场景，并实现"拍照"取得直接证据，从而刷新了人 类对极端天体物理过程的认知。 天文学领域这项突破性的黑洞研究新进展，由中国科学院国家天文台联合郑州大学、香港大学等40 余家高校和科研院所的合作者共同完成，相关论文近日以封面文章形式在最新一期国际学术期刊《科学 通报》（Science Bulletin）发表。 天关卫星科学团队称，此次发现的核心，在于天关卫星搭载有独特而互补的两台X射线望远镜—— 昵称"万星瞳"的宽视场X射线望远镜（WXT）和昵称"风行天"的后随X射线望远镜（FXT）。 0:00 / 1:13 视频来源：中国科学院国家天文台 来自中国科学院国家天文台的最新消息说，天文学家通过对中国天关卫星（爱因斯坦探针，英文缩 写EP）巡天捕获的、编号为EP250702a的高能宇宙爆发事件的最新研究，认为它很可能是一个中等质量 黑洞撕裂并吞噬一颗白矮星的过程。 国际学界对EP250702a事件的起源意见不一，有研究提出，它可能源于恒星质量黑洞与一颗氦星的 并合；有模型考虑恒星级黑洞撕裂普通恒星的可能性。 天关卫星科学团队总结说，EP250702a这一中等质量黑洞以喷流 ...

Core Insights - The detection of gravitational waves by LIGO has opened a new era in gravitational wave astronomy, confirming over a hundred events and validating Stephen Hawking's black hole theory [1][2] - Next-generation detectors like CE, ET, and LISA are in development, promising unprecedented scientific breakthroughs [2][3] Next-Generation Detectors - CE, with a 40 km arm length, aims to detect 100,000 black hole merger events annually, covering the entire history of gravitational wave sources [2] - ET, a European initiative, will extend its frequency range to 1 Hz, allowing earlier detection of black hole collisions and larger mass mergers [2] - LISA, a space-based project, will consist of three satellites forming a triangle of 2.5 million km, targeting low-frequency gravitational waves [2] Technological Innovations - Next-generation detectors incorporate advanced technologies to enhance detection capabilities, such as longer arm lengths for improved sensitivity [3] - Techniques like advanced mirror coatings and low-temperature cooling significantly reduce thermal noise, enhancing detection in the mid-frequency range [3] - Quantum squeezing technology and AI systems are being utilized to suppress noise and improve measurement precision [3] Scientific Potential and Challenges - These detectors hold the potential to explore early universe phenomena, test fundamental physics theories, and advance multi-messenger astronomy [4][5] - They will provide insights into black hole formation, neutron star mergers, and cosmic expansion measurements [4] - However, challenges include noise suppression, precision engineering, and significant funding requirements for projects like ET and LISA [6]