Black Hole - what is that?
A black hole is an astronomical object with a gravitational pull so strong that nothing, not even light, can escape it. A black hole’s “surface,” called its event horizon, defines the boundary where the velocity needed to escape exceeds the speed of light, which is the speed limit of the cosmos. Matter and radiation fall in, but they can’t get out.
Two main classes of black holes have been extensively observed. Stellar-mass black holes with three to dozens of times the Sun’s mass are spread throughout our Milky Way galaxy, while supermassive monsters weighing 100,000 to billions of solar masses are found in the centers of most big galaxies, ours included.
Simulation of hot gas surrounding and falling into a black hole.
(Credit: NASA's Goddard Space Flight Center/J. Schnittman, J. Krolik (JHU) and S. Noble (RIT))
Black Holes
The simplest definition of a black hole is an object that is so dense that not even light can escape its surface. But how does that happen?
The concept of a black hole can be understood by thinking about how fast something needs to move to escape the gravity of another object – this is called the escape velocity. Formally, escape velocity is the speed an object must attain to "break free" of the gravitational attraction of another body.
There are two things that affect the escape velocity – the mass of object and the distance to the center of that object. For example, a rocket must accelerate to 11.2 km/s in order to escape Earth's gravity. If, instead, that rocket was on a planet with the same mass as Earth but half the diameter, the escape velocity would be 15.8 km/s. Even though the mass is the same, the escape velocity is greater, because the object is smaller (and more dense).
What if we made the size of the object even smaller? If we squished the Earth's mass into a sphere with a radius of 9 mm, the escape velocity would be the speed of light. Just a wee-bit smaller, and the escape velocity is greater than the speed of light. But the speed of light is the cosmic speed limit, so it would be impossible to escape that tiny sphere, if you got close enough.
The radius at which a mass has an escape velocity equal to the speed of light is called the Schwarzschild radius. Any object that is smaller than its Schwarzschild radius is a black hole – in other words, anything with an escape velocity greater than the speed of light is a black hole. For something the mass of our sun would need to be squeezed into a volume with a radius of about 3 km.
Structure of a black hole
There are two basic parts to a black hole: the singularity and the event horizon.
The event horizon is the "point of no return" around the black hole. It is not a physical surface, but a sphere surrounding the black hole that marks where the escape velocity is equal to the speed of light. Its radius is the Schwarzschild radius mentioned earlier.
One thing about the event horizon: once matter is inside it, that matter will fall to the center. With such strong gravity, the matter squishes to just a point – a tiny, tiny volume with a crazy-big density. That point is called the singularity. It is vanishingly small, so it has essentially an infinite density. It's likely that the laws of physics break down at the singularity. Scientists are actively engaged in research to better understand what happens at these singularities, as well as how to develop a full theory that better describes what happens at the center of a black hole.
Seeing the unseen
A black hole has two basic parts. The singularity is at the center and is where the mass resides. The event horizon is the boundary that marks where the escape velocity from the mass is the speed of light.
(Credit: NASA's Imagine the Universe)
If light can't escape a black hole, how can we see black holes?
Astronomers don't exactly see black holes directly. Instead, astronomers observe the presence of a black hole by its effect on its surroundings. A black hole, by itself out in the middle of our galaxy would be very difficult to detect.
Imagine you arrive home one night to find the kitchen a mess. You know that it was clean when you left, but now there are dirty dishes in the sink and crumbs strewn about the counter. From the evidence, you know someone used the kitchen while you were out – in fact, you can even say that they made a sandwich and chips because of the types of crumbs you see on the counter. You might even be able to identify who in your household was in the kitchen based on what kind of chips they had or what they put on their sandwich.
You never saw that person in the kitchen, but their effect on the kitchen was evident.
Studying black holes relies heavily on indirect detection. Astronomers cannot observe black holes directly, but see behaviors in other objects that can only be explained by the presence of a very large and dense object nearby. The effects can include materials getting pulled into the black hole, accretion disks forming around the black hole, or stars orbiting a massive but unseen object.
Types of black holes
Traditionally, astronomers have talked about two basic classes of black hole – those with masses about 5-20 times that of the sun, which are called stellar-mass black holes, and those with masses millions to billions times that of the sun, which are called supermassive black holes. What about the gap between stellar mass and supermassive black holes? For a long time astronomers had proposed a third class, called intermediate mass black holes, but it was just in the past decade or so that they have started finding possible evidence of this class of black hole.
Stellar-mass black holes are formed when a massive star runs out of fuel and collapses. They are found scattered throughout the galaxy, in the same places where we find stars, since they began their lives as stars. Some stellar-mass black holes started their lives as part of a binary star system, and the way the black hole affects its companion and their environment can be a clue to astronomers about their presence.
Supermassive black holes are found at the center of nearly every large galaxy. Exactly how supermassive black holes form is an active area of research for astronomers. Recent studies have shown that the size of the black hole is correlated with the size of the galaxy, so that the there must be some connection between the formation of the black hole and the galaxy.
With only a few candidate intermediate black holes, astronomers are just beginning to study them in any detail. These studies are complicated by the fact that many of the objects that initially looked like strong intermediate black hole candidates can be explained in other ways. For example, there is a class of object called ultraluminous X-ray sources (ULXs). These objects emit more X-ray light than known stellar processes. One model postulated that ULXs harbor an intermediate black hole; however, further study of these objects has favored alternate models for most of them.
This image, taken with the European Southern Observatory's Very Large Telescope, shows the central region of galaxy NGC 1313. This galaxy is home to the ultraluminous X-ray source NCG 1313 X-1, which was an intermediate-mass black hole candidate.
(Credit: ESO)
10 Need-to-Know Things About black hole
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Too massive
A black hole is a region in space where the gravitational pull is so strong that nothing, not even light, can escape it.
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One way ticket
The event horizon is the point of no return around a black hole. Once anything crosses the event horizon, it is inevitably pulled into the black hole's singularity.
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Fly and fly
The closest known black hole to Earth is V616 Monocerotis, which is about 3,000 light-years away.
2
Proven by the Theory of Relativity
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Before the explosion
The existence of black holes was first predicted by Albert Einstein's theory of general relativity.
Black holes are formed by the collapse of massive stars.
Singularity is lawlessness
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Different sizes
The singularity is a point of infinite density at the center of a black hole where the laws of physics as we know them break down.
Black holes can range in size from relatively small stellar black holes to supermassive black holes that can have a mass billions of times that of the sun.
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First confirmation!
The first confirmed detection of a black hole was announced in 1971, although the existence of black holes had been theorized for decades before that.
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Breakthrough into the future!
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Not a black hole
Black holes are not actually "black" in the traditional sense; they emit radiation known as Hawking radiation.
The study of black holes has led to some of the most significant breakthroughs in modern physics, including the discovery of the Higgs boson and the development of string theory.