Topic: Research News
The Einstein Probe space telescope detected an unusual X-ray event that may be a black hole tearing apart a white dwarf star. This is the first time this has been observed directly.
On July 2, 2025, the China-led Einstein Probe space telescope spotted an extremely bright X-ray source during its routine survey of the sky. The object's brightness changed rapidly, making it stand out from typical cosmic X-ray sources. This unusual detection prompted observatories around the world to begin follow-up observations.
Researchers from the Department of Physics at The University of Hong Kong helped interpret the observations. Their analysis suggests that the event may represent an intermediate-mass black hole tearing apart and consuming a white dwarf star. If confirmed, it would provide the first direct observational evidence of this type of black hole feeding event.
The discovery relied on the Einstein Probe's two complementary X-ray instruments. The Wide-field X-ray Telescope detected a rapidly changing X-ray source that was later designated EP250702a (also known as GRB 250702B). At nearly the same time, NASA's Fermi Gamma-ray Space Telescope detected several gamma-ray bursts coming from the same region of the sky.
The Einstein Probe's second instrument, the Follow-up X-ray Telescope, then monitored the event as it evolved. Over roughly 20 days, the object's brightness faded by more than a factor of 100,000. During that time, its X-ray emission also shifted from higher-energy (
Implications
The Einstein Probe space telescope detected an unusual X-ray event that may be a black hole tearing apart a white dwarf star. This is the first time this has been observed directly.
Source: https://www.sciencedaily.com/releases/2026/06/260625060222.htm
Journal Reference:
- Dongyue Li, Wenda Zhang, Jun Yang, Jin-Hong Chen, Weimin Yuan, Huaqing Cheng, Fan Xu, Xinwen Shu, Rong-Feng Shen, Ning Jiang, Jiazheng Zhu, Chang Zhou, Weihua Lei, Hui Sun, Chichuan Jin, Lixin Dai, Bing Zhang, Yu-Han Yang, Wenjie Zhang, Hua Feng, Bifang Liu, Hongyan Zhou, Haiwu Pan, Mingjun Liu, Stéphane Corbel, Sitha K. Jagan, Maria Cristina Baglio, Christopher R. Burns, Floriane Cangemi, Chun Chen, Yehao Cheng, Alexis Coleiro, Francesco Coti Zelati, Sourya R. Das, Zhongnan Dong, Luis Galbany, Noa Grollimund, Daniel Kelson, Dong Lai, Xia Li, Yuan Liu, Alessio Marino, Brenna Mockler, Paul O’Brien, Erlin Qiao, Nanda Rea, L. Resmi, Jérome Rodriguez, Richard Saxton, Luming Sun, Lian Tao, Tinggui Wang, Yilong Wang, Xuefeng Wu, Dong Xu, Yijia Zhang, Guoying Zhao, Congying Bao, Zhiming Cai, Yehai Chen, Yong Chen, Bertrand Cordier, Chenzhou Cui, Weiwei Cui, Zhou Fan, He Gao, Giancarlo Ghirlanda, Ju Guan, Dawei Han, Jinxin Hao, Jingwei Hu, Maohai Huang, Yong-Feng Huang, Shumei Jia, Ge Jin, Stefanie Komossa, Chengkui Li, Zhixing Ling, Congzhan Liu, Heyang Liu, Huaqiu Liu, Fangjun Lu, Kirpal Nandra, Jan-Uwe Ness, Arne Rau, Jeremy Sanders, Liming Song, Roberto Soria, Shengli Sun, Xiaojin Sun, Yuyin Tan, Eleonora Troja, Sixiang Wen, Haitao Xu, Changbin Xue, Yongquan Xue, Yi-Han Iris Yin, Chen Zhang, Shuang-Nan Zhang, Yonghe Zhang. A fast powerful X-ray transient from possible tidal disruption of a white dwarf. Science Bulletin, 2026; 71 (3): 538 DOI: 10.1016/j.scib.2025.12.050
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