Chichuan Jin

When a star wanders too close to a black hole, an object with gravity so intense that not even light can escape, tidal forces shred it like dough caught in a mixer's beaters. This event, known as a tidal disruption event (TDE), unleashes a powerful flare of radiation.

At the centers of many galaxies lurk supermassive black holes. From time to time they 'scream' — unleashing powerful X-ray flares. Scientists have long puzzled over the nature of these 'quasi-periodic eruptions'.

A massive star ends its life in a spectacular collapse: the core compresses into a neutron star or a black hole, while the outer layers fly off in a dazzling supernova.

Two glowing embers left over from a fire whirl in the darkness, gradually drawing closer. With each turn, they lose tiny bits of energy that seep into the invisible ripple of space. That is exactly what the system eRASSU J060839.5−704014 looks like — a pair of white dwarfs (superdense stellar remnants) separated by a distance comparable to Earth's diameter.