Are black holes spherical during merger?
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I've been thinking about black holes, specifically during the final moments before two merge. I'm wondering if black holes, or I guess more specifically their event horizons, are always spherical. It seems to me that in the moments before two merge, their respective event horizons will be stretched, somewhat like how the Moon causes our ocean's tides. I have drawn a (poor) diagram of what I think they may look like. Notice how the event horizons are closer to the singularity on the inner side, this is because the gravity from each black hole is in opposition. The event horizons are further from the singularity on the outer side because the gravity from each black hole adds up.
black-hole gravity
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add a comment |
$begingroup$
I've been thinking about black holes, specifically during the final moments before two merge. I'm wondering if black holes, or I guess more specifically their event horizons, are always spherical. It seems to me that in the moments before two merge, their respective event horizons will be stretched, somewhat like how the Moon causes our ocean's tides. I have drawn a (poor) diagram of what I think they may look like. Notice how the event horizons are closer to the singularity on the inner side, this is because the gravity from each black hole is in opposition. The event horizons are further from the singularity on the outer side because the gravity from each black hole adds up.
black-hole gravity
$endgroup$
$begingroup$
Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
$endgroup$
– Steve Linton
May 22 at 7:03
10
$begingroup$
One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
$endgroup$
– Steve Linton
May 22 at 7:07
2
$begingroup$
Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
$endgroup$
– StephenG
May 22 at 14:53
add a comment |
$begingroup$
I've been thinking about black holes, specifically during the final moments before two merge. I'm wondering if black holes, or I guess more specifically their event horizons, are always spherical. It seems to me that in the moments before two merge, their respective event horizons will be stretched, somewhat like how the Moon causes our ocean's tides. I have drawn a (poor) diagram of what I think they may look like. Notice how the event horizons are closer to the singularity on the inner side, this is because the gravity from each black hole is in opposition. The event horizons are further from the singularity on the outer side because the gravity from each black hole adds up.
black-hole gravity
$endgroup$
I've been thinking about black holes, specifically during the final moments before two merge. I'm wondering if black holes, or I guess more specifically their event horizons, are always spherical. It seems to me that in the moments before two merge, their respective event horizons will be stretched, somewhat like how the Moon causes our ocean's tides. I have drawn a (poor) diagram of what I think they may look like. Notice how the event horizons are closer to the singularity on the inner side, this is because the gravity from each black hole is in opposition. The event horizons are further from the singularity on the outer side because the gravity from each black hole adds up.
black-hole gravity
black-hole gravity
edited May 22 at 7:51
Florin Andrei
15.6k1 gold badge40 silver badges54 bronze badges
15.6k1 gold badge40 silver badges54 bronze badges
asked May 22 at 4:07
Ryan_LRyan_L
2682 silver badges6 bronze badges
2682 silver badges6 bronze badges
$begingroup$
Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
$endgroup$
– Steve Linton
May 22 at 7:03
10
$begingroup$
One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
$endgroup$
– Steve Linton
May 22 at 7:07
2
$begingroup$
Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
$endgroup$
– StephenG
May 22 at 14:53
add a comment |
$begingroup$
Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
$endgroup$
– Steve Linton
May 22 at 7:03
10
$begingroup$
One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
$endgroup$
– Steve Linton
May 22 at 7:07
2
$begingroup$
Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
$endgroup$
– StephenG
May 22 at 14:53
$begingroup$
Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
$endgroup$
– Steve Linton
May 22 at 7:03
$begingroup$
Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
$endgroup$
– Steve Linton
May 22 at 7:03
10
10
$begingroup$
One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
$endgroup$
– Steve Linton
May 22 at 7:07
$begingroup$
One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
$endgroup$
– Steve Linton
May 22 at 7:07
2
2
$begingroup$
Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
$endgroup$
– StephenG
May 22 at 14:53
$begingroup$
Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
$endgroup$
– StephenG
May 22 at 14:53
add a comment |
2 Answers
2
active
oldest
votes
$begingroup$
No need to guess. There's solid research done in this field. Even Wikipedia has some info:
As two black holes approach each other, a ‘duckbill’ shape protrudes
from each of the two event horizons towards the other one. This
protrusion extends longer and narrower until it meets the protrusion
from the other black hole. At this point in time the event horizon has
a very narrow X-shape at the meeting point. The protrusions are drawn
out into a thin thread. The meeting point expands to a roughly
cylindrical connection called a bridge.
https://en.wikipedia.org/wiki/Binary_black_hole#Shape
There are research papers with images showing the results of calculations of the shape of the event horizons during merger. Here's an example:
The image above is taken from this paper:
On Toroidal Horizons in Binary Black Hole Inspirals
We examine the structure of the event horizon for numerical
simulations of two black holes that begin in a quasicircular orbit,
inspiral, and finally merge. We find that the spatial cross section of
the merged event horizon has spherical topology (to the limit of our
resolution), despite the expectation that generic binary black hole
mergers in the absence of symmetries should result in an event horizon
that briefly has a toroidal cross section.
$endgroup$
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
$begingroup$
Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
$endgroup$
– Draco18s
May 23 at 2:37
|
show 11 more comments
$begingroup$
From the question What can be learned from, or noted in this LIGO Orrery video? we can watch the video LIGO Orrery (which was inspired by the mind-blowing Kepler Orrery IV).
I've made a small, low quality GIF from screen shots here, the video is much more interesting.
It's been difficult to be sure what exactly is depicted as mentioned in this answer but it's likely the surfaces depict something at least a bit like an event horizon.
$endgroup$
add a comment |
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2 Answers
2
active
oldest
votes
2 Answers
2
active
oldest
votes
active
oldest
votes
active
oldest
votes
$begingroup$
No need to guess. There's solid research done in this field. Even Wikipedia has some info:
As two black holes approach each other, a ‘duckbill’ shape protrudes
from each of the two event horizons towards the other one. This
protrusion extends longer and narrower until it meets the protrusion
from the other black hole. At this point in time the event horizon has
a very narrow X-shape at the meeting point. The protrusions are drawn
out into a thin thread. The meeting point expands to a roughly
cylindrical connection called a bridge.
https://en.wikipedia.org/wiki/Binary_black_hole#Shape
There are research papers with images showing the results of calculations of the shape of the event horizons during merger. Here's an example:
The image above is taken from this paper:
On Toroidal Horizons in Binary Black Hole Inspirals
We examine the structure of the event horizon for numerical
simulations of two black holes that begin in a quasicircular orbit,
inspiral, and finally merge. We find that the spatial cross section of
the merged event horizon has spherical topology (to the limit of our
resolution), despite the expectation that generic binary black hole
mergers in the absence of symmetries should result in an event horizon
that briefly has a toroidal cross section.
$endgroup$
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
$begingroup$
Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
$endgroup$
– Draco18s
May 23 at 2:37
|
show 11 more comments
$begingroup$
No need to guess. There's solid research done in this field. Even Wikipedia has some info:
As two black holes approach each other, a ‘duckbill’ shape protrudes
from each of the two event horizons towards the other one. This
protrusion extends longer and narrower until it meets the protrusion
from the other black hole. At this point in time the event horizon has
a very narrow X-shape at the meeting point. The protrusions are drawn
out into a thin thread. The meeting point expands to a roughly
cylindrical connection called a bridge.
https://en.wikipedia.org/wiki/Binary_black_hole#Shape
There are research papers with images showing the results of calculations of the shape of the event horizons during merger. Here's an example:
The image above is taken from this paper:
On Toroidal Horizons in Binary Black Hole Inspirals
We examine the structure of the event horizon for numerical
simulations of two black holes that begin in a quasicircular orbit,
inspiral, and finally merge. We find that the spatial cross section of
the merged event horizon has spherical topology (to the limit of our
resolution), despite the expectation that generic binary black hole
mergers in the absence of symmetries should result in an event horizon
that briefly has a toroidal cross section.
$endgroup$
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
$begingroup$
Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
$endgroup$
– Draco18s
May 23 at 2:37
|
show 11 more comments
$begingroup$
No need to guess. There's solid research done in this field. Even Wikipedia has some info:
As two black holes approach each other, a ‘duckbill’ shape protrudes
from each of the two event horizons towards the other one. This
protrusion extends longer and narrower until it meets the protrusion
from the other black hole. At this point in time the event horizon has
a very narrow X-shape at the meeting point. The protrusions are drawn
out into a thin thread. The meeting point expands to a roughly
cylindrical connection called a bridge.
https://en.wikipedia.org/wiki/Binary_black_hole#Shape
There are research papers with images showing the results of calculations of the shape of the event horizons during merger. Here's an example:
The image above is taken from this paper:
On Toroidal Horizons in Binary Black Hole Inspirals
We examine the structure of the event horizon for numerical
simulations of two black holes that begin in a quasicircular orbit,
inspiral, and finally merge. We find that the spatial cross section of
the merged event horizon has spherical topology (to the limit of our
resolution), despite the expectation that generic binary black hole
mergers in the absence of symmetries should result in an event horizon
that briefly has a toroidal cross section.
$endgroup$
No need to guess. There's solid research done in this field. Even Wikipedia has some info:
As two black holes approach each other, a ‘duckbill’ shape protrudes
from each of the two event horizons towards the other one. This
protrusion extends longer and narrower until it meets the protrusion
from the other black hole. At this point in time the event horizon has
a very narrow X-shape at the meeting point. The protrusions are drawn
out into a thin thread. The meeting point expands to a roughly
cylindrical connection called a bridge.
https://en.wikipedia.org/wiki/Binary_black_hole#Shape
There are research papers with images showing the results of calculations of the shape of the event horizons during merger. Here's an example:
The image above is taken from this paper:
On Toroidal Horizons in Binary Black Hole Inspirals
We examine the structure of the event horizon for numerical
simulations of two black holes that begin in a quasicircular orbit,
inspiral, and finally merge. We find that the spatial cross section of
the merged event horizon has spherical topology (to the limit of our
resolution), despite the expectation that generic binary black hole
mergers in the absence of symmetries should result in an event horizon
that briefly has a toroidal cross section.
edited May 22 at 7:54
answered May 22 at 7:48
Florin AndreiFlorin Andrei
15.6k1 gold badge40 silver badges54 bronze badges
15.6k1 gold badge40 silver badges54 bronze badges
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
$begingroup$
Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
$endgroup$
– Draco18s
May 23 at 2:37
|
show 11 more comments
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
$begingroup$
Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
$endgroup$
– Draco18s
May 23 at 2:37
15
15
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
$begingroup$
+1 Lovely pictures. I appreciate how the xyz-axes in the corners contribute absolutely nothing.
$endgroup$
– user28113
May 22 at 14:16
12
12
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
$begingroup$
@user28113 The coordinates make sense in the context of the simulation described in the paper. These are the actual results of numeric analysis - not "an artist's impression" of the phenomenon.
$endgroup$
– Florin Andrei
May 22 at 17:59
8
8
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
$begingroup$
@WhitePrime Black holes are basically just powerfully distorted spacetime. At the singularity our math blows up so it's pointless to talk much about that. The event horizon is the boundary where things get different in many ways - but it's not a line drawn in the sand, nor is it a "solid object". It's more like the Equator - you know it's there, you can measure and calculate it, but there is no white line on the ground that says "Equator". The shape of the event horizon is influenced by rotation, other massive bodies nearby, etc. It would be spherical for a static, isolated black hole.
$endgroup$
– Florin Andrei
May 22 at 19:57
6
6
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
$begingroup$
@WhitePrime They do, yes. But rubber balls are not the only things that can "wobble". Spacetime itself can wobble. Particles in a magnetic trap could wobble. Entire universes could wobble if conditions are right. "Wobbling" simply means there's a force that opposes a deformation, and it brings the system back to the initial point, but it overshoots and is deformed in the opposite direction, and then it's brought back again, etc. Many things can do this.
$endgroup$
– Florin Andrei
May 22 at 22:26
5
5
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Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
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– Draco18s
May 23 at 2:37
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Square smoke rings wobble. As for the boundary that is called the event horizon, it is simply the demarcation of a region of space inside of which we, being on the outside, cannot assign a "when" to any event that occurs on the inside. Stuff happens in there, but we'd need to wait an infinite amount of time to see it.
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– Draco18s
May 23 at 2:37
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show 11 more comments
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From the question What can be learned from, or noted in this LIGO Orrery video? we can watch the video LIGO Orrery (which was inspired by the mind-blowing Kepler Orrery IV).
I've made a small, low quality GIF from screen shots here, the video is much more interesting.
It's been difficult to be sure what exactly is depicted as mentioned in this answer but it's likely the surfaces depict something at least a bit like an event horizon.
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add a comment |
$begingroup$
From the question What can be learned from, or noted in this LIGO Orrery video? we can watch the video LIGO Orrery (which was inspired by the mind-blowing Kepler Orrery IV).
I've made a small, low quality GIF from screen shots here, the video is much more interesting.
It's been difficult to be sure what exactly is depicted as mentioned in this answer but it's likely the surfaces depict something at least a bit like an event horizon.
$endgroup$
add a comment |
$begingroup$
From the question What can be learned from, or noted in this LIGO Orrery video? we can watch the video LIGO Orrery (which was inspired by the mind-blowing Kepler Orrery IV).
I've made a small, low quality GIF from screen shots here, the video is much more interesting.
It's been difficult to be sure what exactly is depicted as mentioned in this answer but it's likely the surfaces depict something at least a bit like an event horizon.
$endgroup$
From the question What can be learned from, or noted in this LIGO Orrery video? we can watch the video LIGO Orrery (which was inspired by the mind-blowing Kepler Orrery IV).
I've made a small, low quality GIF from screen shots here, the video is much more interesting.
It's been difficult to be sure what exactly is depicted as mentioned in this answer but it's likely the surfaces depict something at least a bit like an event horizon.
answered May 24 at 1:11
uhohuhoh
9,7743 gold badges26 silver badges88 bronze badges
9,7743 gold badges26 silver badges88 bronze badges
add a comment |
add a comment |
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Relevant if not an exact dupe is the last point in astronomy.stackexchange.com/questions/28610/…
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– Steve Linton
May 22 at 7:03
10
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One problem with this question is that, by definition, a black hole is a place where space and time are quite distorted and things are generally happening rather quickly. So simply asking what shape the event horizons are at a particular moment is not really a well-defined question. Defining which events are happening at the same time is a somewhat arbitraru process depending on the observer, while defining "shape" meaningfully needs quite a bit of differential geometry. The SXS simulations (black-holes.org) make an attempt and you can read their papers for the details.
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– Steve Linton
May 22 at 7:07
2
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Even single black holes that have non-zero angular momentum (that "rotate") have non-spherical "shapes".
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– StephenG
May 22 at 14:53