Swift Summary
- The black hole M87, located 55 million light-years from Earth at the center of galaxy Messier 87, has shown unexpected changes in its magnetic field as observed over three images captured in 2017, 2018, and 2021 by the Event Horizon Telescope (EHT) collaboration.
- These changes were visible in polarized light and include a “flip” of the magnetic field’s polarization pattern between images taken across these years.
- Scientists attribute this variability to potential shifts in the underlying magnetic field structure, changes in Faraday rotation effects, dynamic regions near the black hole like plasma disks or jets, or a combination of these factors.
- M87 is massive – more than six billion times the mass of our Sun – and its environment plays a key role in galaxy evolution by influencing star formation and energy distribution through powerful matter jets that travel at nearly light speed.
- The EHT’s new findings trace how polarization reveals fluctuations in matter states around M87, providing insights into black hole accretion processes.
Indian opinion Analysis
The changing nature of M87‘s environment underscores ongoing advancements in astrophysical research technology. India’s own growing space ambitions could gain inspiration from such international collaborations like EHT to expand on domestic astrophysics capabilities. Further studies on supermassive black holes have implications for understanding broader cosmic phenomena like galaxy evolution – an area where India can leverage initiatives like ISRO’s Astrosat mission. Strengthening research partnerships with global institutions such as Max Planck Institute may enhance India’s theoretical frameworks related to relativistic physics and observational astronomy.
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