Detection Methods Detection Astrophysical Phenomena Black Hole Mergers Space-Time Black Holes LISA Mission Supermassive Black Holes Binary Systems Research Methods Observatories Astrophysics Cosmic Phenomena Gravitational Wave Background Low-frequency Gravitational Waves Origins Theoretical Foundations Confirmation of Einstein's Theory Research Collaboration Frequency Range Low-Frequency Gravitational Waves Ultra-low Frequency Gravitational Waves Types Sources Research Accretion Disks Observational Astronomy Observational Techniques Mass Transfer Cosmic Events LISA LISA Spacecraft LISA Observatory Black Hole Dynamics Space-Time Distortions Ultralow Frequency Gravitational Waves Cosmic History Frequency Analysis Black Hole Interactions Neutron Stars Detection Techniques Formation High-Frequency Gravitational Waves LIGO Detectors Research Techniques LIGO Statistical Techniques Merging Black Holes Wave Spectrum Dark Matter
A rare tidal disruption event, AT2024tvd, has revealed a supermassive black hole 2,600 light-years from its galaxy's center, challenging assumptions about their locations.