The Accidental Astrophysicists
An anonymous reader recommends a ScienceNews story that begins: "Dmitry Khavinson and Genevra Neumann didn't know anything about astrophysics. They were just doing mathematics, like they always do, following their curiosity. But five days after they posted one of their results on a preprint server, they got an email that said 'Congratulations! You've proven Sun Hong Rhie's astrophysics conjecture on gravitational lensing!'... Turns out that when gravity causes light rays to bend, it can make one star look like many. But until Khavinson and Nuemann's work, astrophysicists weren't sure just how many. Their proof in mathematics settled the question."
Mathematics results are physically relevant. News at 11.
The wikipedia article on gravitational lensing has a neat animation produced with a numerical model. I wouldn't make it your desktop background though because it might warp your file icons.
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OMFG! It's full of stars!
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n refers to the number of massive objects causing the lensing as I understand it, but I could be wrong. I'm slightly drunk while posting and my previous existence as an astronomy grad student eludes me.
Clearly n is the fudge factor.
... that xkcd is right: http://xkcd.com/435/
Three is my favourite number
There's something I don't understand here. If n > 1, the number of images is 5n-5, or 5(n-1). As n must be an integer (You can't have a fraction of a massive object.) that means that the number of images must be a multiple of 5. And yet, there's a picture of a set of 4 images of a quasar in the article. Not only that, somebody links to the Wikipedia article on gravitational lensing, and that shows a picture of an "Einstein Cross:" four images of a quasar surrounding a galaxy between it and us. Four, in both cases, not five. Yes, I realize that in both cases n = 1, but can anybody explain how you end up with four in that case?
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I think the article says that this equation is used to find the maximum amount of star images that could be created by a massive object, so in the case of one massive object, according to the equation, you could get a maximum of 5 images of the star.
n = # of massive objects in the way, not light sources.
I'm not actually an astrophysicist, but I may be able to sort of explain. Take a look at the diagram in TFA: it's just in two dimensions, specifically the plane defined by the distant star, the massive object, and the observer. We see two images that are in that plane, because only light rays from the star that are traveling in that plane can be bent by the massive object so that they can reach us; rays traveling in any other plane would be bent to arrive at some other location. And the star is effectively a point source, so we see exactly two point images. With multiple massive objects, there are more planes, but the planes are still discrete, so there are still discrete images. The only exception is when the star, the massive object, and the observer are exactly in line, in which case we see a circle.
Galaxies, on the other hand, are not point sources, which is why when we see gravitationally lensed galaxies they often look stretched out along arcs -- different points in the galaxy line up differently, and thus can look farther apart from each other than they would if we were seeing them without lensing.
So the number you see doesn't have to be a multiple of 5 always, even for n>1.
There's no guarantee that you can see the 'straight through' image, because the object doing the lensing might be in the way.
And for n objects lensing, the effect is multiplicative.
What's so difficult about that?
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