In the cluster Abell 2218 (pictured here), distant blue galaxies behind the large
cluster of galaxies are "squished" into a circular shape around the
middle of the foreground cluster. This is from gravitational lensing.
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The possibility that the path of light could be bent by the gravity of a large object was predicted by Einstein's Theory of General Relativity, and this effect was observed soon after the theory was published. Because people normally think of glass or plastic lenses as bending light, we call any massive object that bends light rays a "gravitational lens." By measuring the amount of bending, we can then determine the mass of whatever is doing the bending.
In the cluster Abell 2218 (pictured here), distant blue galaxies behind the large
cluster of galaxies are "squished" into a circular shape around the
middle of the foreground cluster. By measuring the amount of
distortion in the more distant blue galaxies, we can determine the mass of the cluster. In fact, we can even
measure how much mass there is that we can't see -- this galaxy
cluster happens to have nearly 400 trillion times the sun's mass in
"dark" matter.
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A relatively new method used by astronomers is to look for a change in the way light behaves, due to gravitational lensing. It is somewhat akin to how you avoid running through sliding glass doors. If the glass is very clean and you get no reflections, how can you tell the door is there? Your eyes perceive that the light from outside is bent, and infer that something is bending it, namely the door. Note that you didn't see light FROM the door, but you saw the effect made by the door on light from objects behind it. Similarly, we can use telescopes to look at light from very distant objects behind the clusters of galaxies we are interested in to study the clusters. The possibility that the path of light could be bent by the gravity of a large object was predicted by Einstein's Theory of General Relativity, and this effect was observed soon after the theory was published. Because people normally think of glass or plastic lenses as bending light, we call any massive object that bends light rays a "gravitational lens." Astronomers now use specialized electronic cameras on large telescopes to very carefully measure how much the light from background objects is bent. By analyzing the amount of bending, we can then determine the mass of whatever is doing the bending.
In the cluster Abell 2218, distant blue galaxies behind the large
cluster of galaxies are "squished" into a circular shape around the
middle of the foreground cluster. By measuring the amount of
distortion in the more distant blue galaxies, we can determine that
there is indeed "dark" matter in the cluster! In fact, we can even
measure how much mass there is that we can't see -- this galaxy
cluster happens to have nearly 400 trillion times the sun's mass in
"dark" matter.
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Page created January 4, 2006 by Travis Metcalfe.
Last modified July 23, 2008 by Randy Russell.
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