Supermassive Black Holes Formation Tidal Disruption Events Accretion Disks Primordial Black Holes Intermediate-Mass Black Holes Characteristics Quasars Implications Gravitational Waves Supermassive Black Hole M87* Massive Black Holes Stellar-Mass Black Holes Observations Event Horizon Telescope Galaxies Growth Milky Way Black Hole Mergers Black Hole Growth Stellar Black Holes Distant Black Holes Black Hole Formation Tidal Disruption Events (TDEs) Dormant Black Holes Research Methods Active Galactic Nuclei Mergers Event Horizon Oldest Black Hole Black Hole Activity Consequences Formation of Black Holes Types of Black Holes Accretion Disk Research Studies Research Active Black Holes Stellar-mass Black Holes Accretion Discs Galaxy Evolution Luminosity Black Hole Environment Magnetic Fields Stellar Evolution Properties Future Observations Simulations Detection Study Methods Challenges Technology Jets Sagittarius A* Intermediate-mass Black Holes Milky Way Galaxy Intermediate-Size Black Holes Jet Formation Detection Methods Types Comparison Jet Movement Galactic Mergers Future Implications SS 433 Early Universe Black Holes Magnetic Field Study Black Hole Properties Observation Techniques Mass Gap NASA Visualization Black Hole Effects Black Hole Outflows Relativistic Jets Black Hole Phenomena Medium-Sized Black Holes Exciting Aspects Galaxy Importance Black Hole Size Comparative Analysis Particle Beams Light Emission NASA Smaller Black Holes Observational Methods Black Hole Shadows Gravity Mass Black Hole Feeding Microquasars Jet Reorientation Jet Direction Falling Process Conditions Active Galactic Nuclei (AGN) Interferometric Imaging Magnetic Structure
Analysis of 2021 VLBI data links the black hole’s ring to a compact radio region about 0.09 light-years from M87*.
