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haileyparikh
I've been reading 'A brief history of time' and want to know more about how black holes are formed. Please help?
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haileyparikh said:I've been reading 'A brief history of time' and want to know more about how black holes are formed. Please help?
This is not accurate. When stars get too big, they don't collapse, they explode: the nuclear forces overwhelm gravity at the radius of even the most densely packed star. Only the core gets crushed enough to turn into a black hole, and it's not simply gravity doing that. Gravity keeps the hole collapsed, but the momentum of the rest of the star falling onto the core is what crushes it into a hole.Abullais Ghazi said:When the escape velocity of a star becomes extremely high then it starts consuming itself or starts degrading itself and a time comes when their is no existence of star at that place but there is a very high concentration of Gravitational force at that point and finally it starts attracting everything even light! I hope you got the answer.
I think your attempt to simplify the explanation of "what is a black hole" is just making it more confusing. You make it sound like magic, whereas it is a well understood physical process and no, there are not "millions of conflicting theories"Abullais Ghazi said:I simply want to say that when the escape velocity of that star exceeds the velocity of light then there is a formation of black hole takes place. I want to end my answer in simple language other wise it takes a lot of problem to the questioner. You are throwing light on the stages of black hole. The stellar nebula first becomes the massive star then in the red super giant then into supernova and then either in black hole or in neutron star. There millions of conflict on theories of black hole and even on there existence. Everyone wants to explain the fundamentals of black hole in his own way. Researches are still going on but still we are unaware of a extremely vast part of universe...
Isn't this the definition of the event horizon? Isn't a black hole escape velocity >= c?Chronos said:Any region of space where the escape velocity = c, is a black hole by definition.
This description isn't accurate, either.newjerseyrunner said:This is not accurate. When stars get too big, they don't collapse, they explode: the nuclear forces overwhelm gravity at the radius of even the most densely packed star. Only the core gets crushed enough to turn into a black hole, and it's not simply gravity doing that. Gravity keeps the hole collapsed, but the momentum of the rest of the star falling onto the core is what crushes it into a hole.
That works with stars in the 10 to ~130 solar mass range, or stellar remnants with a combined mass greater than ~3 solar masses (such as the collision of two neutron stars). However, once you get stars that are greater than ~130 solar masses the temperature, pressure and gamma-rays from the collapsing core it is sufficient to create electron-positron pairs, which annihilate each other. The thermal energy released by the electron-positron pairs overcomes the gravitational binding energy of the core and the core also explodes, leaving nothing behind. So like neutron stars, which have a range between 1.44 and ~3 solar masses, black holes also appear to have a minimum and maximum range with regard to stellar remnants. Obviously another mechanism, other than a stellar core collapse, is required to produce black holes greater than ~39 solar masses.SteamKing said:This description isn't accurate, either.
When a massive star reaches the end of its life, its core is no longer capable of using nuclear fusion to create enough energy to support itself against gravity wanting to collapse it further. When fusion ceases, gravity wins the battle and collapse occurs rather suddenly. As the collapsing core gets denser and denser, eventually a point is reached in some stars where the core cannot collapse further, and it stops abruptly. The envelope of the star, having rushed into fill the void left by the collapse of the core, strikes the surface and rebounds. The shock wave created by the rebound is sufficient to blow the star's envelope into space, leaving the neutron star core behind:
https://en.wikipedia.org/wiki/Type_II_supernova
If the core is sufficiently massive, when collapse occurs, there will be no rebound, and a black hole will be created:
https://en.wikipedia.org/wiki/Black_hole
Sometimes, even if a dead star leaves a neutron star behind, this star can collect enough additional mass from surrounding gas to collapse into a black hole.
It's also possible for two neutron stars to collide and, because their combined mass is so great, only a black hole is left behind.
Since supermassive's seem to all be at the heart of galaxies, it seems very reasonable that they grew from scratch by accreting new material from the very dense area at the center of the galaxy. First enough to create a BH and then more until they had cleared out a large area around them (small fraction of the galaxy's diameter but a good sized volume in absolute terms).|Glitch| said:Obviously another mechanism, other than a stellar core collapse, is required to produce black holes greater than ~39 solar masses.
Neon said:A black hole IS actually just a 'hole' in the fabric of the universe
Well, It will be easier to imagine gravity with the universe as a fabric. I read it somewhere,couldn't remember.davenn said:do you have a reference for that ummm interesting comment ?
How come popular literature writes "nothing can escape, not even light". Light does travel at c, doesn't it? Or is, perhaps, my conception of c at fault here, then?Chronos said:Any region of space where the escape velocity = c, is a black hole by definition.
He meant >cnuuskur said:How come popular literature writes "nothing can escape, not even light". Light does travel at c, doesn't it? Or is, perhaps, my conception of c at fault here, then?
Neon said:He meant >c
nuuskur you are also right too.
So if i reach Earth's escape velocity exactly, i will not get out of earth? exclude friction.davenn said:no he meant c meaning light DOESNT escape
Neon said:A black hole IS actually just a 'hole' in the fabric of the universe
nuuskur said:What makes the black hole have such intense gravity? Is it correct to think a black hole is made of compacted matter?
nuuskur said:How does that look like exactly? Are the elementary particles, neutrons, protons, electrons smashed together?
nuuskur said:If so, isn't there a limit for how "dense" a black hole could get, yet we speak of black holes and then Supermassive black holes, quasars and whatnot.
There is no "fabric of the universe", that's just a pop-sci type description that is badly overused.Neon said:A black hole IS actually just a 'hole' in the fabric of the universe and is black as no light escapes it. Creation of a black hole is more complex depending on the mass of the star of other stuff.
"I read it somewhere" is not a valid citation for this site. We all forget where we read things, but when you are defending something that is pop-science, not actual science, you need to do better.Neon said:Well, It will be easier to imagine gravity with the universe as a fabric. I read it somewhere,couldn't remember.
Neon said:Well, It will be easier to imagine gravity with the universe as a fabric. I read it somewhere,couldn't remember.
phinds said:There is no "fabric of the universe", that's just a pop-sci type description that is badly overused.
"I read it somewhere" is not a valid citation for this site. We all forget where we read things, but when you are defending something that is pop-science, not actual science, you need to do
Neon said:I am talking about that.Took me a while to find it. If you find what i said eailer confusing.
As i said, it makes it easier tovisualizeNeon said:Well, It will be easier to imagine gravity with the universe as a fabric. I read it somewhere,couldn't remember.
You don't need any general relativity or exotic science for that. Just take a look at Newton's centuries-old law for classical gravitational attraction, ##F=Gm_1m_2/r^2##. There are two ways of making ##F## greater: make one or both masses larger; or make ##r## smaller. For example, gravity at the surface of the Earth is what it is because the radius of the Earth is about 6400 kilometers; if we took the same mass and squished it down into a radius of 3200 kilometers while keeping the mass the same, the gravitational force at the new surface closer to the center would be four times as great.nuuskur said:What makes the black hole have such intense gravity?
Most of the space inside a back hole (that is, the space inside the event horizon which is what we generally think of as the surface of the black hole) is actually vacuum. All of the matter is concentrated in a very small area (general relativity says it's a point of zero size, but that just tells us that even the theory of GR isn't accurate under those extreme conditions and we need some new physics) at the center; as Drakkith says, we have no idea what's going on there,and we won't until we figure out some new physics.Is it correct to think a black hole is made of compacted matter?
That is the result that we get if we take the Einstein Field Equations at face value. Everything inside the event horizon must end up at the central singularity. It is impossible for anything to remain in the region of spacetime "between" the event horizon and the central singularity, for about the same reason that I cannot remain at 12:00 noon today - like it or not, I'm going to move from 12:00:00 to 12:00:01.stewart brands said:Is it not true that within the event horizon of a so called Black Hole,the mass is confined to an extradinarily small space relative to other mass distributions everywhere else?
Is it not true that there is so much mass confined that the pressure forces cause limited degrees of freedom for the atoms such that massive amounts of heat derived from atomic motion is dissipate?
Is it not also true that the models go further and describe the elimination of all electrons and the nucleii themselves disassociate into their constituents(bosons subsequent to fermion ejection)?
Is it not true then that this degree of freedom starved mass of energy would have very little heat and be extremely cold?
The question that now follows is :would this mass have the properties and nature of a Bose-Einstein Condensate with very small S / entropy?
If not how would the two states differ?
If the nucleus of a Black Hole is not cold then why not?
If the entropy in this domain does shrink in an extraordinarily unique way then does that mean the bosons travel faster within this medium than they ordinarily would/(compared to a laboratory Bose-Einstein Condensate)?
If they conserve the second law with heat of motion then waht happens if the confinement becomes so great that they must exceed or almost exceed c to conserve the heat?
SteamKing said:Sometimes, even if a dead star leaves a neutron star behind, this star can collect enough additional mass from surrounding gas to collapse into a black hole.
It's also possible for two neutron stars to collide and, because their combined mass is so great, only a black hole is left behind.
Bernie G said:Not so. The most massive neutron star which has been observed is about 2 solar masses. The smallest black hole observed is about 5 solar masses. Draw your own conclusions.
Bhs smaller than 5 sm are possible.Those bh are so light than few clues are released ( x ray...) so maybe in the future we will find super light bhs.SteamKing said:There may be BHs which are smaller than 5 solar masses, but we just haven't observed them. There's no violation of any fundamental physics laws if smaller BHs exist.
Two neutron stars have been shown in simulation to merge into a single object which forms a BH.
http://www.iflscience.com/space/what-happens-when-neutron-stars-collide
Black holes are formed when a massive star dies and collapses under its own gravity. As the star runs out of fuel, it can no longer produce enough energy to counteract the force of gravity, causing it to collapse in on itself. This creates a singularity, a point of infinite density and zero volume, at the center of the black hole.
Black holes cannot be directly observed, but their presence can be inferred through their effects on surrounding matter. Scientists use various methods, such as observing the gravitational lensing of light from distant stars, to detect the presence of black holes. Additionally, the detection of gravitational waves, ripples in space-time, can also provide evidence of black holes.
The size of a black hole is determined by its mass. The more mass a black hole has, the larger its event horizon, the point of no return for anything that enters it. The smallest black holes are known as stellar black holes and can have a mass equivalent to a few times that of our sun. Supermassive black holes, on the other hand, can have a mass equivalent to billions of suns.
Contrary to popular belief, black holes do not suck everything in. Their gravitational pull is only strong enough to capture objects that come within a certain distance, known as the event horizon. Anything that passes beyond the event horizon is unable to escape, but objects that are far enough away can still orbit the black hole without being pulled in.
Black holes are not inherently dangerous, but they can be destructive to anything that gets too close. As objects enter the event horizon, they are stretched and torn apart by the immense gravitational forces. However, the chances of encountering a black hole in space are extremely low, and they pose no threat to Earth or our solar system.