After an extensive two-decade observation effort, astrophysicists have confirmed that a supermassive black hole residing at the center of a nearby galaxy is indeed spinning, providing substantial support for Albert Einstein’s enduring theories of general relativity. The study, published on September 27, utilized images from observatories around the Earth to reveal that the black hole’s jet, which consists of streams of particles emanating from the void’s axis, was in motion, solidifying the conclusion that the black hole is spinning.
This supermassive black hole is situated around 55 million light-years away in the heart of the nearby Messier 87 galaxy, also known as M87. The study disclosed that the black hole’s jet follows a predictable 11-year cycle, ultimately enabling scientists to confirm its rotation.
The astrophysical community has been closely monitoring whether supermassive black holes rotate, making this discovery a significant milestone. Spin is one of the two primary properties attributed to astrophysical black holes, the other being mass. It has historically been challenging to measure the spin of black holes. Hence, this finding provides essential independent evidence supporting the notion that the black hole in M87 is indeed spinning.
Confirming the rotational nature of supermassive black holes aligns with Einstein’s theories of relativity, further establishing these theories on a more robust footing. Wystan Benbow, an astrophysicist at the Harvard-Smithsonian Center for Astrophysics, emphasized that independently corroborating black hole spin using this novel technique advances various crucial theories in astrophysics.
The supermassive black hole in M87 is an astonishing 5.4 billion times more massive than the Sun and holds the distinction of being the first black hole ever photographed. Before this revelation, scientific knowledge was based primarily on circumstantial evidence of spinning black holes. However, the latest discovery furnishes compelling proof of this phenomenon.
This breakthrough is pivotal in the world of astronomy, as it has implications for understanding the symbiotic evolution of black holes and their host galaxies and offers insights into the formation of the universe’s large-scale structure.
Black holes, especially supermassive ones, are ubiquitous and reside at the centers of nearly all galaxies. This revelation about the spinning nature of the black hole at the heart of the M87 galaxy is a significant milestone in the ongoing quest to decipher the mysteries of the cosmos.
Disclaimer: The views, suggestions, and opinions expressed here are the sole responsibility of the experts. No Science Currents journalist was involved in the writing and production of this article.