Philip Kaaret

In 1936, two physicists, Werner Heisenberg and Hans Euler, poring over the equations of quantum electrodynamics, found something strange. In a sufficiently strong magnetic field, vacuum should cease to be empty.

In the binary system Cyg X-2, a neutron star pulls matter from a normal companion star. The infalling gas spirals in, heats up to millions of degrees, and shines brightly in X-rays. Astronomers pointed two space telescopes, IXPE and NuSTAR, at this object and, for the first time, measured in detail how polarized that light is.

The edge of the supernova remnant RCW 86 is where the shock wave from a star's explosion slams into the surrounding gas. The IXPE telescope looked at the southwestern part of this boundary in X-rays and tried to catch polarization — the way these rays oscillate.

The black hole GS 1354-64 in the constellation Musca woke up in 2025 and began greedily pulling matter from its companion star. The orbiting X-ray telescope IXPE caught it at a rare moment: the outburst had already subsided, but the system had not yet settled down.

Deep in space, a rapidly spinning neutron star, a pulsar nicknamed the Lighthouse, speeds through tenuous gas. Like a motorboat cutting through water, it leaves a glowing trail of charged particles behind. In X-rays, this trail appears as a bright tail and a thin filament stretching over many light-years.