Currently, sci.esa.int is under review and not being updated. For the latest information and news from ESA science missions and scientific results, please visit esa.int. For a comprehensive overview of ESA’s Science Programme and its missions, please refer to science.esa.int. For in-depth technical information aimed at ESA's scientific communities, you may also wish to consult cosmos.esa.int.

Asset Publisher

Back Artist's impression of radio bursting magnetar

Artist's impression of radio bursting magnetar


Date: 28 July 2020
Satellite: INTEGRAL
Copyright: ESA

Artist's impression of SGR 1935+2154, a highly magnetised stellar remnant, also known as a magnetar.

Discovered in 2014 in the constellation of Vulpecula following a substantial burst of X-rays, the magnetar became active again in April 2020. ESA's Integral high-energy space observatory detected a burst of high-energy, or 'hard', X-rays on 28 April, automatically alerting observatories worldwide about the discovery in just seconds. Soon after, astronomers spied something astonishing: this magnetar was not only radiating its usual X-rays, but radio waves, too.

This unique mix of radiation, never before seen bursting from such a stellar remnant, may solve a long-standing cosmic mystery about the nature of Fast Radio Bursts – powerful events that pulse brightly in radio waves for just a few milliseconds before fading away, and are only rarely seen again.

Last Update: 28 July 2020
14-Jun-2026 16:31 UT

ShortUrl Portlet

Shortcut URL

https://sci.esa.int/s/wV2gMEw

Related Images

Related Videos

Related Publications

Related Links

Documentation