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.
... that xkcd is right: http://xkcd.com/435/
Three is my favourite number
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.
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.