M87 Black Hole: Spinning at Near Light Speed
- Scientists have obtained new measurements of the supermassive black hole at the center of the M87 galaxy, determining its spin and accretion rate with unprecedented accuracy.
- The Event Horizon Telescope's iconic images provided the data for this fresh look.
- The team analyzed the "shining spot" in the original images, a phenomenon caused by relativistic Doppler beaming.This effect makes material moving toward us appear brighter.Measuring this brightness difference...
Scientists have precisely measured the spin and accretion rate of the supermassive black hole at the heart of the M87 galaxy. The findings reveal this behemoth spins at an remarkable 80% of the theoretical maximum speed, confirming its extreme nature. Material plunges into the black hole at 23% the speed of light. The study, leveraging data from the Event Horizon Telescope, also details the black hole’s consumption rate, offering fresh insights into its behavior and the powerful jets it fuels. News Directory 3’s coverage of this discovery offers a window into the cutting edge of astrophysics. Discover what future investigations will uncover about this cosmic giant and its influence on the universe.
M87 Black Hole’s Spin and Accretion Rate Precisely Measured
Updated June 9, 2025
Scientists have obtained new measurements of the supermassive black hole at the center of the M87 galaxy, determining its spin and accretion rate with unprecedented accuracy. The findings reveal the extreme nature of this cosmic object, one of the largest known black holes in our galactic neighborhood.
The Event Horizon Telescope’s iconic images provided the data for this fresh look. Researchers calculated that the black hole, boasting a mass 6.5 billion times that of the sun, spins at approximately 80% of the theoretical maximum speed. Material at the inner edge of its accretion disk whips around at roughly 14% the speed of light, or 42 million meters per second.
(Image credit: Hubble Space Telescope)
The team analyzed the “shining spot” in the original images, a phenomenon caused by relativistic Doppler beaming.This effect makes material moving toward us appear brighter.Measuring this brightness difference allowed scientists to determine the black hole’s rotation speed.
Furthermore, the study examined magnetic field patterns, revealing that matter spirals into the black hole at about 70 million meters per second, or 23% the speed of light. Based on these measurements,scientists estimate that M87’s black hole consumes between 0.00004 and 0.4 solar masses of material annually. While significant, this is relatively modest for such a massive black hole, indicating it operates below the Eddington limit in a quieter phase.
The results are pretty mind-blowing. This black hole, which weighs in at 6.5 billion times the mass of our Sun, is spinning at roughly 80% of the theoretical maximum speed possible in the universe.
Crucially, the energy from infalling material aligns with the power output of M87’s prominent jet, a beam of particles extending thousands of light-years at near light-speed. This supports the theory that the black hole’s feeding process fuels these powerful jets.
What’s next
Future telescopes and advanced imaging promise even greater insights into M87’s black hole, offering a cosmic laboratory to test our understanding of gravity, spacetime, and extreme physics. These measurements will help answer fundamental questions about how these cosmic entities shape galaxies and influence the universe’s fate.