G. Ramsay

On the night of August 18, 2025, the SVOM space telescope detected a short gamma-ray burst — a powerful flash of energy lasting less than two seconds. Such bursts are usually linked to mergers of neutron stars, the ultra-dense remnants of dead stars.

A hot star in its death throes trembles like a plucked string. Its surface oscillates with amplitudes of thousandths of a magnitude, like noticing a light bulb in a room flicker 0.3% brighter. For a space telescope, such precision is routine, but from Earth, the atmosphere gets in the way.

Two hundred and eighty-nine days: that's how long one rotation of the white dwarf white dwarf WD 1532+129 takes. This is not just a record: on its surface, near the magnetic poles, scars of iron and other metals appear — silent testimony to planets it has devoured.