Table of Contents
- 1 Why does the accretion disk around a black hole look warped?
- 2 Why can we see light from the accretion disk even if it’s on the back side of the black hole?
- 3 How do each of the three types of black holes form?
- 4 How does a black hole warp space?
- 5 Are black holes discs or spheres?
- 6 How do black holes look like?
- 7 How supermassive black holes are formed?
- 8 What is an accretion disc in a black hole?
- 9 Why is one side of a black hole brighter than another?
- 10 Do supermassive black holes exert gravity towards anything other than themselves?
Why does the accretion disk around a black hole look warped?
This left only one possible explanation, the huge X-ray flux was irradiating the disk and causing it to warp. The warp provides a huge increase in the area of the disk that could be illuminated, thereby making the visual light output increase dramatically when viewed at the right time.
Why can we see light from the accretion disk even if it’s on the back side of the black hole?
Supermassive black holes have such an intense gravitational pull that they bend light right around them, allowing us to see an “echo” of the side that would otherwise be hidden from view.
Can we see the accretion disk of a black hole?
Although no-one has ever actually seen a black hole or even its event horizon, this accretion disk can be seen, because the spinning particles are accelerated to tremendous speeds by the huge gravity of the black hole, releasing heat and powerful x-rays and gamma rays out into the universe as they smash into each other …
How do each of the three types of black holes form?
There are four types of black holes: stellar, intermediate, supermassive, and miniature. The most commonly known way a black hole forms is by stellar death. As stars reach the ends of their lives, most will inflate, lose mass, and then cool to form white dwarfs.
How does a black hole warp space?
“The reason we can see that is because that black hole is warping space, bending light and twisting magnetic fields around itself.” According to Einstein’s theory of general relativity, massive objects warp the fabric space-time. That, Einstein said, is gravity.
Why do black holes look like that?
Bottom right: Approaching the black hole, gravity is so strong that light is severely bent, creating a bright (almost circular) ring. Gravitational lensing magnifies the apparent size of the black hole’s event horizon into a larger dark shadow.
Are black holes discs or spheres?
A black hole is a sphere in the sense that everything that goes within its Schwarzschild radius (the distance from the center of the black hole to the event horizon) cannot escape its gravity. Thus, there is a dark sphere around the infinitely dense center, or singularity, from which nothing can escape.
How do black holes look like?
Black holes have gravitational fields so strong that even light cannot escape, so they are defined by the shell of a black, featureless sphere called an event horizon. But the holes can nevertheless be seen. The black hole bends light around it, creating a circular shadow.
What color is a black hole accretion disk?
The gas swirls in an accretion disk surrounding the black hole, thus heating up and emitting radiation. Ultimately, the gas falls into the black hole and contributes to its mass. Theories predict that the spectrum of the radiation emitted from the accretion disk is mostly blue.
How supermassive black holes are formed?
One possible mechanism for the formation of supermassive black holes involves a chain reaction of collisions of stars in compact star clusters that results in the buildup of extremely massive stars, which then collapse to form intermediate-mass black holes.
What is an accretion disc in a black hole?
An accretion disc is stuff orbiting around the black hole as it is falling into it. Or it would be possible that the particles are in some sort of orbit around the black hole. This disc would be outside of the event horizon so it isn’t really “in” the black hole.
Where does the distortion occur in a black hole?
The greatest distortion occurs when viewing the system nearly edgewise. 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.
Why is one side of a black hole brighter than another?
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.
Do supermassive black holes exert gravity towards anything other than themselves?
It would seem that supermassive black holes only exert gravity towards themselves. When it comes to accretion disks, nothing is coming out of the black hole. That’s just orbiting matter, though it is swirled around a bit by frame dragging. Even at high gravity, the ability to orbit around a massive body still exists.