Near-Perfect Einstein Ring Discovered
Fraser Cain writes "Universe Today is reporting on the discovery of a nearly perfect Einstein Ring; a gravitational lens of a nearby galaxy working as a natural telescope to focus the light from a more distant galaxy. Gravitational lenses have been seen many times before, but never so complete, with a close lensing galaxy and a distant magnified galaxy."
Well, this is a nice discovery to celebrate the 100 years of the Einstein's miraculous year and 50 years since the guy passed away.
See, now they have a really good reason to get up there and maintain Hubble. I mean seriously, what better reason than to focus hubble on that Einstein ring and get a very upclose view of a distant galaxy
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If we can see that universe better, the opposite is true, they can see us better.
That being said, I want to be the first to welcome our new voyeuristic overlords.
It's seven billion lightyears away! The article specifically notes that the great distance makes it even more special.
And because it's so far away, while still in focus, we can look back further than ever before. It'll be interesting to see some theories about the early universe shattered to pieces.
The official scientific term for gravitational lensing that produces a ring image is an "Einstein ring". The submitter/editors didn't make it up; it's right in the title of the paper.
Well that seems to be relatively obvious and maybe insignificant compared to what can be done just by improving the receiving setup.
So I thought, if we increase our telescope resolution to the point where we can get a very high resolution image of the 11 bn ly galaxy, and find a perfect Einstein ring in that, might it not be then possible to find an even farther (say 20 bn ly galaxy) that might by fabulous luck be lined up with it, and thereby (luck again) piggy back all the way up to the end of visible space?
So question 1) If we had a 1 AU wide telescope and enough Einstein rings, just how far do you think we could really see?
This sounds similar to the idea of pointing a big telescope at the edge of a black hole to view the entire universe (since light can orbit many times before leaving, at least according to a neat story called the Planck Dive). So 2) assuming the black holes or something close enough to them really exist in our galaxy, what could such a large telescope reveal by focusing on the edge of such a black hole, and 3) is there any way possible to use one possibly in conjunction with piggy backed Einstein rings to see light beyond what is the "visible universe" i.e. the point at which expanding space has expanded beyond our light cone.
It would seem that an image that had been captured by a black hole before much expansion had occurred could conceivably be accessible now (if black holes truly can be "read" that way not just in fiction) even though the space being imaged has long expanded far beyond the edge of the visible universe. IANA astronomer but interested in where fact and fiction separate and neat ways to use computer graphic techniques and telescopes. Can anybody experienced answer some of these questions?
They sure did ... they power supply ran off of coffee, food, and oxygen, and they required at least 8 hours of downtime a day for them to function properly [and to prevent overheating]. The results they produced were displayed on dead tree paste that was flattened and gathered together in groups.
And then mathematicians and physicists would use the results of these computations instead of wasting time computing things like the square root of 3021377 by hand.
Something a lot less worthwhile?
Of course that does not solve the issue of needing to maintain the new telescope
Actually, it goes a long way towards that goal. By discovering that parts X, Y, and Y are prone to breaking on the Hubble, those parts can be redesigned for a new model to be much more break resistant and longer lasting.