Six panel illustration of Black Hole TDE AT2024tvd

This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 
1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 
2) A wayward star gets swept up in the black hole's intense gravitational pull; 
3) The star is stretched or "spaghettified" by gravitational tidal effects;
4) The star's remnants form a disk around the black hole; 
5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells.

Six panel illustration of Black Hole TDE AT2024tvd

This six-panel illustration of a tidal disruption event around a supermassive black hole shows the following: 
1) A supermassive black hole is adrift inside a galaxy, its presence only detectable by gravitational lensing; 
2) A wayward star gets swept up in the black hole's intense gravitational pull; 
3) The star is stretched or "spaghettified" by gravitational tidal effects;
4) The star's remnants form a disk around the black hole; 
5) There is a period of black hole accretion, pouring out radiation across the electromagnetic spectrum, from X-rays to radio wavelengths; and 6) The host galaxy, seen from afar, contains a bright flash of energy that is offset from the galaxy's nucleus, where an even more massive black hole dwells.

https://science.nasa.gov/asset/hubble/six-panel-illustration-of-black-hole-tde-at2024tvd/