Explanation:
If one black hole looks strange, what about two? Light rays from accretion disks around a pair of orbiting supermassive black holes make their way through the warped space-time produced by extreme gravity in this detailed computer visualization. The simulated accretion disks have been given different false color schemes, red for the disk surrounding a 200-million-solar-mass black hole, and blue for the disk surrounding a 100-million-solar-mass black hole. For these masses, though, both accretion disks would actually emit most of their light in the ultraviolet. The video allows us to see both sides of each black hole at the same time. Red and blue light originating from both black holes can be seen in the innermost ring of light, called the photon sphere, near their event horizons. In the past decade, gravitational waves from black hole collisions have actually been detected, although the coalescence of supermassive black holes remains undiscovered.
https://www.nasa.gov/universe/new-nasa-visualization-probes-the-light-bending-dance-of-binary-black-holes/
https://apod.nasa.gov/apod/ap200825.html
https://en.wikipedia.org/wiki/Accretion_disk
https://apod.nasa.gov/apod/ap190411.html
https://svs.gsfc.nasa.gov/14132/
https://ui.adsabs.harvard.edu/abs/1993AmJPh..61..619N/abstract
https://apod.nasa.gov/htmltest/rjn_bht.html
https://en.wikipedia.org/wiki/Photon_sphere
https://apod.nasa.gov/apod/ap201104.html

https://apod.nasa.gov/apod/ap250506.html

#space #blackhole #astrophotography #photography #astronomy #science #nature#NASA#ESA

Credit: NASA’s Goddard Space Flight Center
Jeremy Schnittman (NASA/GSFC)
Scott Wiessinger (USRA)
Francis Reddy (University of Maryland College Park)
Francis Reddy (University of Maryland College Park)

This new visualization of a black hole illustrates how its gravity distorts our view, warping its surroundings as if seen in a carnival mirror. The visualization simulates the appearance of a black hole where infalling matter has collected into a thin, hot structure called an accretion disk. The black hole’s extreme gravity skews light emitted by different regions of the disk, producing the misshapen appearance.

Bright knots constantly form and dissipate in the disk as magnetic fields wind and twist through the churning gas. Nearest the black hole, the gas orbits at close to the speed of light, while the outer portions spin a bit more slowly. This difference stretches and shears the bright knots, producing light and dark lanes in the disk.

Viewed from the side, the disk looks brighter on the left than it does on the right. Glowing gas on the left side of the disk moves toward us so fast that the effects of Einstein’s relativity give it a boost in brightness; the opposite happens on the right side, where gas moving away us becomes slightly dimmer. This asymmetry disappears when we see the disk exactly face on because, from that perspective, none of the material is moving along our line of sight.

Closest to the black hole, the gravitational light-bending becomes so excessive that we can see the underside of the disk as a bright ring of light seemingly outlining the black hole. This so-called “photon ring” is composed of multiple rings, which grow progressively fainter and thinner, from light that has circled the black hole two, three, or even more times before escaping to reach our eyes. ...

>> https://svs.gsfc.nasa.gov/13326

#space #blackhole #astrophotography #astrophysics #photography #astronomy #science #nature#NASA

As our viewpoint rotates around the black hole, we see different parts of the fast-moving gas in the accretion disk moving directly toward us. Due to a phenomenon called "relativistic Doppler beaming," gas in the disk that's moving toward us makes that side of the disk appear brighter, the opposite side darker. This effect disappears when we're directly above or below the disk because, from that angle, none of the gas is moving directly toward us.

When our viewpoint passes beneath the disk, it looks like the gas is moving in the opposite direction. This is no different that viewing a clock from behind, which would make it look like the hands are moving counter-clockwise.

CORRECTION: In earlier versions of the 360-degree movies on this page, these important effects were not apparent. This was due to a minor mistake in orienting the camera relative to the disk. The fact that it was not initially discovered by the NASA scientist who made the movie reflects just how bizarre and counter-intuitive black holes can be!

Credit: NASA’s Goddard Space Flight Center
Jeremy Schnittman (NASA/GSFC)
Scott Wiessinger (USRA)
Francis Reddy (University of Maryland College Park)
Francis Reddy (University of Maryland College Park)

>>https://svs.gsfc.nasa.gov/13326#section_credits

#space #blackhole #astrophysics #astrophotography #photography #astronomy #science #nature#NASA#ESA

I’m an #actuallyautistic #disabledartist, living in lutruwita/Tasmania, #australia, in my mid 30s. I specialise in #landscapephotography, #astrophotography, and #timelapse in the island’s wild places.

I like to play with light. These are some of my more successful experiments.

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