galaxy M87 on a scale below that expected for its event horizon. Pictured, the dark central region is not the event horizon, but rather the black hole's shadow -- the central region of emitting gas darkened by the central black hole's gravity. The size and shape of the shadow is determined by bright gas near the event horizon, by strong gravitational lensing deflections, and by the black hole's spin. In resolving this black hole's shadow, the Event Horizon Telescope (ETH) bolstered evidence that Einstein's gravity works even in extreme regions, and gave clear evidence that M87 has a central spinning black hole of about 6 billion solar masses. The EHT is not done -- future observations will be geared toward even higher resolution, better tracking of variability, and exploring the immediate vicinity of the black hole in the center of our Milky Way Galaxy.
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NASA Official: Jay Norris. Specific rights apply.
A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
Based on Astronomy Picture Of the Day
Publications with keywords: black hole
Publications with words: black hole
- The Milky Way s Black Hole
- First Horizon Scale Image of a Black Hole
- EHT Resolves Central Jet from Black Hole in Cen A
- GW200115: Simulation of a Black Hole Merging with a Neutron Star
- Animation: Black Hole Star Shredder
- The Doubly Warped World of Binary Black Holes
- The Galaxy, the Jet, and a Famous Black Hole