Skip to main content
Admissions guidance, study banks, and career tools — get started on Shalyam
Research News

Astronomers Witness Birth of a Powerful Magnetar (2)

Mayur Tembhare
  1. Astronomers detected an X-ray flash that lasted 10 minutes, which might be the birth of a magnetar.

  2. The event was detected by the Einstein Probe satellite on July 4, 2025.

  3. Neutron stars are extremely dense objects left behind when massive stars die.

  4. Magnetars are rapidly spinning neutron stars with huge magnetic fields.

Astronomers Witness Birth of a Powerful Magnetar (2)

Topic: Space

Researchers detected an X-ray flash that lasted 10 minutes. They think it might be the birth of a magnetar, a powerful object created when two neutron stars collide.

Astronomers have long used brief bursts of gamma rays to find collisions between neutron stars. These flashes are very short-lived, disappearing in less than two seconds. Now, new research suggests that some neutron star mergers may also produce X-ray flashes that last much longer.

The study was published in Science Bulletin and presents strong evidence for this connection. The researchers used data from the Einstein Probe satellite, which has detected hundreds of bright X-ray flashes from distant galaxies since its launch in January 2024. These events are called fast X-ray transients and have several possible origins. Some are connected to massive stars dying, while others remain unexplained.

The team led by Professor Eleonora Troja's group obtained observations that helped identify the source of one such X-ray transient. They used several instruments, including the European Southern Observatory's Very Large Telescope (VLT) and the Very Large Array. By studying what remained after the explosion, they concluded that they may have witnessed the formation of a magnetar produced by the collision of two neutron stars.

Neutron stars are extremely dense objects left behind when massive stars die. When two neutron stars merge, they generate gravitational waves that travel through space. The light produced during these events can help astronomers determine what survives the collision.

Why It Matters

This discovery helps us understand how powerful objects like magnetars are formed in the universe. It also shows how scientists use advanced technology to study distant events and learn more about the cosmos.

Key Facts

  • Astronomers detected an X-ray flash that lasted 10 minutes, which might be the birth of a magnetar.
  • The event was detected by the Einstein Probe satellite on July 4, 2025.
  • Neutron stars are extremely dense objects left behind when massive stars die.
  • Magnetars are rapidly spinning neutron stars with huge magnetic fields.

Key Terms

neutron star
An extremely dense object left behind when a massive star dies.
magnetar
A powerful object created when two neutron stars collide, characterized by its rapid spin and huge magnetic field.
gamma-ray burst
A brief burst of gamma rays that can be used to find collisions between neutron stars.

Implications

This discovery helps us understand how powerful objects like magnetars are formed in the universe. It also shows how scientists use advanced technology to study distant events and learn more about the cosmos.

Source: https://www.sciencedaily.com/releases/2026/09/260930020252.htm

Journal reference:

  1. An Li, Chen-Wei Wang, Niccolò Passaleva, Jie An, Bin-Bin Zhang, Eleonora Troja, Yi-Han Iris Yin, Yuan Liu, Shao-Lin Xiong, Li-Ping Xin, Yi-Xuan Shao, Jun Yang, Hui Sun, Dong Xu, Yu-Han Yang, Roberto Ricci, He Gao, Sarah Antier, Rosa L. Becerra, Jia-Xin Cao, Alberto Javier Castro-Tirado, Xin-Lei Chen, Ye-Hao Cheng, Yong Chen, Hua-Qing Cheng, Valerio D’Elia, Massimiliano De Pasquale, Yong-Wei Dong, Eslam Elhosseiny, Rob A.J. Eyles-Ferris, Maria Gritsevich, Xu-Hui Han, Dieter Hartmann, You-Dong Hu, Jing-Wei Hu, Shu-Mei Jia, Nino Kochiashvili, Wei-Hua Lei, Andrew J. Levan, Cheng-Kui Li, Dong-Yue Li, Hua-Li Li, Xiao-Bo Li, Zhi-Xing Ling, He-Yang Liu, Hou-Jun Lü, Daniele B. Malesani, Brendan O’Connor, Hai-Wu Pan, Shashi Bhushan Pandey, Ignacio Perez-Garcia, Daniëlle L.A. Pieterse, Marion Pillas, Yu-Lei Qiu, Andrea Saccardi, Rubén Sánchez-Ramírez, Wen-Jun Tan, Manasanun Tanasan, Nial R. Tanvir, Susanna D. Vergani, Jing Wang, Xiao-Feng Wang, Qin-Yu Wu, Shu-Xu Yi, Tillayev Yusufjon, Chen Zhang, Wen-Da Zhang, Yi-Jia Zhang, Guo-Ying Zhao, Chao Zheng, Shi-Jie Zheng, Chang Zhou, Ping Zhou, Bertrand Cordier, Jian-Yan Wei, Weimin Yuan, Shuang-Nan Zhang, Bing Zhang. Minutes-long soft X-ray prompt emission from a compact object merger. Science Bulletin, 2026; 71 (18): 4657 DOI: 10.1016/j.scib.2026.08.021

Leave a comment

← All research

Get Exclusive Insights with Every Issue

Join Shalyam Newsletter

Stay ahead in education, research, and innovation—straight to your inbox.