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Wants to develop a space telescope that can study gamma-ray bursts from black holes

Black hole.
Published Apr 01, 2025

Black holes have long fascinated humans and sparked curiosity about the cosmos and science. Black holes are created when a massive star collapses; its birth is revealed as an intense flash of gamma rays in the sky. Mark Pearce, professor of physics at KTH Royal Institute of Technology, wants to develop a cutting-edge gamma-ray space telescope to study how black holes are created in the universe and how a huge amount of energy is released.
"Gamma-ray bursts are the most energetic explosions in the universe, releasing as much energy in a few seconds as the sun generates in a billion years," he says.

Measurements will have a higher diagnostic value

The telescope will consist of electronic X-ray detectors and X-ray optics. A unique feature will be able to determine the degree of polarisation of gamma rays, which means that measurements will have significantly higher diagnostic value than is possible with today's telescopes.

Parts of the technology have previously been developed at KTH and tested in space using huge research balloons launched from the Esrange space station outside Kiruna. The next step would be to use a small satellite to carry out observations over a much longer period from orbit.

"It would be very exciting to tackle big scientific questions using a national infrastructure," says Mark Pearce.

One of the challenges in developing the space telescope is developing technology compatible with a small satellite. The technology must be compact, have low mass and power, generate manageable amounts of data, and withstand the severe vibrations during launch and the temperature fluctuations in orbit.

The extreme physical environment around a black hole, such as high temperature and gravity, means that it is possible to study how matter and radiation behave in a way that is not possible on Earth.

"Discoveries in basic research have benefited society in the past in ways that are very difficult to predict," says Mark Pearce.

Mark Pearce.

The technology must be compact

Gamma-ray astrophysics is a very active field of research, and today, Mark Pearce and his colleagues are collaborating with groups in several locations around the world. And thanks to the research already done at KTH on balloon-borne instrumentation, expertise has been built up in measuring the polarisation properties of gamma rays.

"Being able to measure the polarisation of gamma-ray bursts means that a space telescope from KTH would be groundbreaking and unique in the research landscape," says Mark Pearce.

Mark Pearce

Mark Pearce is a Professor of Astroparticle Physics and develops instruments and methods to study cosmic rays from space. His research focuses on X-ray polarimetry, a new observational method for studying celestial sources.

Mark Pearce's research contributes to new knowledge about black holes and rotating neutron stars, known as pulsars. Among other things, Mark has led the development of the custom-built PoGO+ telescope from KTH Royal Institute of Technology, which has collected crucial data on the supernova remnant Crab Nebula and the black hole Cygnus X-1. He has also led Sweden's contribution to XL-Calibur, a new 12-metre-long space telescope weighing around two tonnes, which lifted off this summer from Esrange in Kiruna using a helium-filled balloon larger than the Globe. The new advanced telescope can measure the energy and polarisation of X-rays even more accurately than before, providing valuable new insights into black holes and pulsars.