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Astronomers Observe Unprecedented X-Ray Flashes from Distant Black Hole

A white dwarf star orbiting near the event horizon of a supermassive black hole may explain unusual X-ray variability and rapid acceleration.

Overview

  • Researchers from MIT and international institutions observed accelerating X-ray flashes from the black hole 1ES 1927+654, located 236 million light-years away in the Draco constellation.
  • The flashes increased in frequency from every 18 minutes in 2022 to every seven minutes by 2024, a phenomenon never seen before in such rapid progression.
  • Scientists suggest a white dwarf star is orbiting dangerously close to the black hole, shedding mass and stabilizing its inward motion near the event horizon.
  • The black hole's activity has been monitored since 2018, including the disappearance and reappearance of its X-ray-emitting plasma corona and the launch of ionized gas jets in 2024.
  • Future gravitational wave detectors like ESA's LISA, expected to launch in the 2030s, may confirm the presence of the white dwarf and provide further insights into this rare system.