Why does light bend around a massive object if spacetime bends inward?

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flyerpower
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I'm having some troubles understanding how spacetime actually looks and what causes gravity and unifying the idea with the general relativity consequences, like light bending.

So, if spacetime is bent by massive objects like in this picture:
Illustration of Earth surrounded by a grid of curved lines bending toward it across a starfield, representing spacetime warped by mass; a bright blurred star appears in the lower right corner.


HOW does the light bend outwards that massive object like in this picture :

Artist's diagram of gravitational lensing: light from a distant galaxy at upper right curves around a foreground galaxy cluster and reaches an observer at lower left, with a central lensing mass and a small blue-haloed Earth shown.


Shouldn't it bend inwards if the spacetime lines are pointing inwards the object?
If the spacetime looks like in the first picture is very easy how to figure out where the gravity comes from.
 
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  • Earth drawn in the centre of a starfield, with a grid of curved pale lines bending inward around it, illustrating curved spacetime; a bright glowing sphere appears at the lower right.
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Ultimately, you cannot understand general relativity by hoping to look at pictures and see how spacetime "bends". The only way to do that is to look at and understand the equations.

At any rate, it's much easier if you move the problem down into two dimensions (So you can use the third two denote curvature, i.e. the bowling ball on a rubber sheet analogy). Then it should appear fairly obvious to you why the light rays behave how they do in the 2nd picture.
 
Nabeshin said:
Ultimately, you cannot understand general relativity by hoping to look at pictures and see how spacetime "bends". The only way to do that is to look at and understand the equations.

At any rate, it's much easier if you move the problem down into two dimensions (So you can use the third two denote curvature, i.e. the bowling ball on a rubber sheet analogy). Then it should appear fairly obvious to you why the light rays behave how they do in the 2nd picture.

Well, i don't have yet the necessary math knowledge to understand the equations, so I'm just trying to understand the concept.

If i look at the curvature in two dimensions the light bending is obvious for me, but the gravity doesn't, that would mean the gravity force would not point to the center of the earth.
 
Ultimately 4-dimensional spacetime curvature cannot be visualized, we can only talk so much about imagining a curved 2-dimensional surfaces etc. but it is not the real thing. All these analogies really don't teach you much other than give you a very rough idea (which will break down if you try to go into the details of the analogy too much)

Three-panel comic: a stick figure lecturer says space-time is like a rubber sheet that massive objects distort, then pauses 'Wait.' A student at a desk asks 'They distort it because they're pulled down by... what?' A third figure sighs. The lecturer, at a blackboard of equations, says the analogy must be an approximation, then 'Booooring.'
 
flyerpower said:
I'm having some troubles understanding how spacetime actually looks and what causes gravity and unifying the idea with the general relativity consequences, like light bending.

So, if spacetime is bent by massive objects like in this picture:
Illustration of Earth in space with curved grid lines drawn around it, bending inward toward the planet, with a bright glowing object at lower right against a starry background.


HOW does the light bend outwards that massive object like in this picture :

Diagram of gravitational lensing: a distant galaxy at upper right, a large foreground galaxy cluster in the centre, a smaller dark lensing body, and Earth at lower left, with light paths curving around the foreground mass.


Shouldn't it bend inwards if the spacetime lines are pointing inwards the object?
If the spacetime looks like in the first picture is very easy how to figure out where the gravity comes from.
I don't understand your question. In both pictures, the lines are bending inward, not outward.
 
flyerpower said:
HOW does the light bend outwards that massive object like in this picture :

Diagram of gravitational lensing: light rays from a distant galaxy bend around a large foreground galaxy cluster and converge on Earth, with a small inset galaxy and background stars.


Shouldn't it bend inwards if the spacetime lines are pointing inwards the object?
Actually the picture does not show light bending outwards.

Remember that the light leaves the nebula from all directions! All rays in the picture bend towards the gravitating object.
 
Passionflower said:
Actually the picture does not show light bending outwards.

Remember that the light leaves the nebula from all directions! All rays in the picture bend towards the gravitating object.

Probably you are referring to the earth, i meant the object between the Earth and the source of light.
 
flyerpower said:
Probably you are referring to the earth, i meant the object between the Earth and the source of light.

I think we are still somewhat confused. The light also bends inward (note the curvature is *toward* not *away*) the object between Earth and source of light. The white curve denotes the light ray that would have otherwise go in straight line but bent *inward* by its gravity instead and therefore towards Earth.
 
Oh, now i see, i didn't pay much attention to what Passionflower said
Remember that the light leaves the nebula from all directions! All rays in the picture bend towards the gravitating object.

Thanks.
 
jambaugh said:
lol! Beautifully perfect cartoon... Where did you find it??

xkcd :-)
 
How I found to "visualize" it is to firstly not ignore time. I imagine (with one less spatial dimension) a central mass as a (heavy) line in the t direction. Then imagine fluid flow (its velocity representing reciprocal of clock ticks for an array of clocks around the mass). The central mass slows down clocks (spreading out ticks and thus shorter reciprocal ticks). Now imagine other objects being sheared inward toward the central mass as lines refracting toward slower time.

Use relativity of simultaneity to arbitrarily match up parallel ticks as a spatial surface (with time-like normal) and notice how as you propagate forward to later ticks the normal turns inward. I'll work up a diagram and post it in a bit.
 
jambaugh said:
How I found to "visualize" it is to firstly not ignore time.
See also related discussion and links in this post:
https://www.physicsforums.com/showthread.php?p=2046692&postcount=4


jambaugh said:
I imagine (with one less spatial dimension) a central mass as a (heavy) line in the t direction. Then imagine fluid flow (its velocity representing reciprocal of clock ticks for an array of clocks around the mass). The central mass slows down clocks (spreading out ticks and thus shorter reciprocal ticks). Now imagine other objects being sheared inward toward the central mass as lines refracting toward slower time.

That is a way to get 2 + 1 spacetime in a 3d picture. Instead of embedding curved 2 space or 2 + 1 spacetime in 3d, we can represent intrinsic curvature as varying density of spacetime. Then we can use the analogy between the worldlines of freefallers in that spacetime and a laser beam in a medium of varying optical density. Both are bend towards the denser area. With two spatial dimensions and time we can visualize orbits, by a laser beam spiraling around a denser column in the medium.

And if we use the propertime as the time dimension, we can even visualize gravitational by a laser that advances slower along that dimension, when going trough a denser area.