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We’ve talked about gravitational lensing before. You know what that is; it’s when light is bent in response to the gravitational pull of an object of respectable mass. Say you’re looking at a very distant light source, like a galaxy. If there is a massive object between you and the light source (like a massive planet), you will see the light bent around the object — it looks like a distortion in your telescope.
It’s not a distortion… it’s something that was discussed way back in 1924 (Orest Chwolson) and 1912 (Albert Einstein). This effect wasn’t scientifically proven until 1979. It’s scary sometimes to think about how smart these people were, you know? How great it would be to have Einstein or Galileo in modern times. Think what they could do with our telescopes today.
Anyway, one very interesting thing about the lensing we’re seeing today is that we see light bending around some massive source of gravity that we can’t see. It’s not black holes (we’re getting good at pinpointing those), and they don’t think there’s a massive planet there… it’s just light reacting to something we haven’t seen yet. Wow. Could it be dark matter, you think? Something else?
The distortion effect is called Einstein Rings, and I did a post on them a while back. You can read it here if you’d like.
Basically, light will move in a fairly straight path away from it’s source unless it’s acted upon, either by a source of gravity, warps in the fabric of space-time, or something else. You know light consists of tiny, discrete packages of photons; it exists as a wave-particle duality that can be influenced and acted upon. Gravitational lensing is when you see light being influenced. Isn’t that cool? That’s particle physics, and I know you guys love your physics!
Studies from the lensing in the Hubble ST images has even given scientists a rough idea of the location of “something else” in the visible star field. Here’s what the 3D image of it looks like:
This is believed to be the location of dark matter. Of course, nobody can prove that’s what it is yet, but it’s not anything else we’ve seen so far. Mostly because nothing else except gravitational lensing can “see” it. Something’s there, and it has mass.
The field is still young, and there’s no telling what we’ll find with it in the future, or in what direction the field will take us. It’s wide open; waiting for you to fill in the blanks.
In the meanwhile, we get this:

Posted September 6, 2010
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