Huge Lenses To Observe Dark Energy
Iddo Genuth writes "UK astronomers, as a part of the Dark Energy Survey collaboration, have reached a milestone in the construction of one of the largest ever cameras to detect dark energy by completing the shipment of the glass required for the five special lenses. Each step in the process of completing this sophisticated camera brings scientists closer to detecting the invisible matter that cosmologists estimate makes up around 75% of our universe."
They're making it sound like dark energy is visible light. If it's "dark" that means it's undetectable by normal means like giant lenses for instance. How could you just see dark energy? Isn't it more like something you'd detect with sensors, not a giant lense? But no, straight out of the article, they're gonna use it to for "detecting the invisible matter" because it has "advanced optics." Btw they said MATTER, not energy so apparently that's what they're actually looking for. Well that would officially make it dim matter, wouldn't it? Like I always thought, dark matter is just matter without a whole lot of light shining on it cuz it's in between galaxies and stuff.
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Narrative: Somewhere on a distant planet
Astronomer "Did you see that flash, hah proof dark energy doesn't exist"
I know that planets aren't considered dark matter but I always wonder if the scientists out there are taking into account all the planets and asteroids out there that we cant see. I mean every other day, it seems, I'm reading about new gas giant planets detected around distant suns and the articles always make out as if its a surprise to the guys who found it. Is it possible that we might have underestimated the amount of planetary debris that we just can't see with current telescopes?
"I see nothing... nothing!" Yup, must be dark energy out there.
Dark energy may be an indicator that we live in a false vacuum. If this is the case and the true vacuum is speeding towards us with the speed of light then we are doomed. So, add another doomsday scenario to your list.
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Are you sure you removed the world's largest lens cap.
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scientists needing huge optics 8-) whood a thought it
sorry for my comments, I'm drunk
I did not find TFA very illuminating. Of course the topic was optically sensing the effects of Dark Energy which doesn't radiate, so maybe I wasn't supposed to be illuminated.
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Basically, they will take more accurate measurements than before. Then they will look at how badly gravity-only models fail. They will adjust this as much as possible using the imaginary qualities of "dark matter". When they still come up well short of getting it right, then the rest will be explained away by assuming "dark energy" wherever needed to adjust for the failure.
When "96% of the universe" is only detectable by how your model fails with the visible stuff alone, measurements of the visible stuff become useless. It isn't even science at that point.
Freedom is assumed. Then they try to take it away. The degree to which you resist is the degree to which you are free.
But for many years the biggest mirror was the 200-inch Hale Telescope at Palomar Mountain near San Diego. Nowadays there are several monolithic 8-metre mirrors, and the two 10-meter Keck telescopes atop Mauna Kea, Hawaii; they are composed of carefully aligned hexagonal subsections.
Why the big disparity?
With a lens, you have to grind and polish both sides, and what's worse, a single lens won't do because all glass refracts different colors differently, giving rise to chromatic aberration. A minimum of two lenses is required, for four surfaces to fabricate.
For both lenses and mirrors, the tolerance of the surface is a small fraction of a wavelength of light across the whole surface. But for lenses, all the surfaces must also be very accurately parallel.
But really the worst problem is that with a lens, the light goes through the thickness of the glass. The glass must therefore be very uniform and free of internal stresses that could alter the index of refraction in different places.
Such glass is very difficult to make; no doubt these lenses are only possible because of recent advances in optical glass manufacture.
That's not a problem for mirrors; observatory telescopes use "first-surface" mirrors, which are aluminized on the front, so the light doesn't go through the glass. Mirror glass therefore doesn't need such careful tolerances.
But my guess is that they are using lenses because they have a much wider field of view; it's quite easy to make a lens with a sixty degree field of view, but with a mirror the field of view is typically a fraction of a degree. With small amateur scopes, the maximum field is about a degree, twice that of the full moon.
That seems clear from the photo, because of the steep curvature of the glass; wide-angle lenses usually have very strong curves.
And yes, I know what I'm talking about - I'm an avid amateur telescope maker, and at one time was a Caltech astronomy student. I've published in the Astrophysical Journal, and have done observing runs at the Palomar 60 and 200 inch telescopes.
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Occam's Razor actually works against MOND. MOND has to be changed to account for what we observe at pretty much every scale. The MOND that works for Galaxy rotation doesn't work for clusters, which doesn't work for lensing, which doesn't work for early structure formation, and so on.
LCDM accounts for this. Heck, you don't think that we scientists got together one day and said "I know, lets make up some goofy theory and then fudge the data to fit it!" do you? You do realize multiple theories were purposed, predictions were created, new data was taken, and conclusions drawn about which theories were supported by the new evidence, right? And that LCDM is the one that survived all the vetting?
Just checking... See, that's sort of how science is supposed (and did in this case) work.
Well, it doesn't mean that the lens sees it, but that the lens can see the effect it has on the things you _can_ see. For instance you look at a galaxy field and you notice that some are distorted in certain ways, you can infer that there's a hidden mass between you and those galaxies. The LSST project on which I work has a similar goal.
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As for the other, Occam's Razor has little to do with logic per se. Rather, it implies that the simplest solution (i.e., the one that introduces fewest complications) is the most likely to be correct.
Actually it says that the solution requiring the fewest assumptions is the one most likely to be correct. The correct solution could still be more complex (which is my assumption on what you mean by complications) than other proposed solutions. When the number of assumptions is equal then the solution with the lower complexity is favoured.
The tyrant will always find a pretext for his tyranny - Aesop
That's somewhat incorrect, and makes a hash of two unrelated things too:
1. Dark matter. Unlike what its name might imply, it isn't dark as in "light absorbing". It's dark as in, it doesn't interact with light at all, except through gravity.
It's only "dark" in the same way as a sheet of glass is dark against the night sky.
But even that metaphor is misleading. "Dark matter" is just a name for a lot of mass that should be there according to calculations (or our understanding of gravity is completely broken at large scales), but hadn't been observed. It's just a funky name. It doesn't mean it's actually dark in any form or shape.
The best example of a scale where this is visible is inside a galaxy. With just gravity determining the speed of rotation around the centre, the stars closer to the centre should rotate faster than those on the edges. (In the same way as Mercury rotates around the sun once every 0.24 years, Earth in a year, and Pluto in 248 years.) But galaxies don't seem to rotate that way. They rotate more like a solid texture, so to speak. So there must be some mass distributed through the disc, in addition to what we see.
But again, the whole point is that we can't see it. If it were just a cloud of pitch-black baryonic matter, that would actually be easy and comfortable. We'd just do what you said: look at what happens to the light of stars behind it. Since it's plenty of it inside a galaxy, we have plenty of stars to look at and notice if something like that was between us and them. But all we can see is some extra gravity, with all that involves for both star movement and gravitational lensing.
A much more accurate name would be "completely transparent matter."
2. Dark energy.
This is an even funnier concept. With all that mass in the universe, there's gravity all around. Duly noted, the gravity pull of a hideously distant galaxy is really tiny, but it's there. The universe expansion should slow down as gravity pulls everything towards the centre. The funny thing is: it doesn't. It's actually accelerating, and weirdly enough, the farther something is, the faster it seems to accelerate away.
There is _something_ that pushes stuff away from the centre, and it's not like any force we already know.
It's also something we'd be hard pressed to reproduce in a lab. Whatever it is, it's insignificantly weak at small ranges, and only starts to matter at very very very large distances. Even at galactic scales (hundreds of thousands at light years) it seems to do practically nothing at all, but move a few _billion_ light years away, and you start seeing whole galaxies accelerating away. It's not something you can reproduce in a lab.
It's also weird in that a normal energy (e.g., the potential energy in a compressed spring) would get used up, or rather converted into work, as it pushes stuff away. So the force would logically diminish. This one only seems to grow stronger.
So basically this big "WTF?" is what's called "dark energy". There's some energy that's pushing the universe apart, but we don't know what it is, and how to detect it.
A polar bear is a cartesian bear after a coordinate transform.
In that respect it's completely different from iron oxidation.
The other way is to overcoat it with something tough and transparent; traditionally silicon monoxide was used.
One can both protect the aluminum and enhance its reflectivity by giving it multiple layers of tough, transparent minerals. Interference effects cause it to reflect better than aluminum would alone.
That's how laser mirrors work - they're not aluminized. It's the same principle as antireflective coatings on camera and eyeglass lenses, but a different choice of refractive indices and thicknesses causes it to enhance rather than cancel reflections.
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When "96% of the universe" is only detectable by how your model fails with the visible stuff alone, measurements of the visible stuff become useless. It isn't even science at that point.
I'd say it is. I'm under the impression, that dark matter & energy hypothesis (I think it's fair to call it a hypothesis at this point) is the simplest explanation for all the observations that we have. So I'd say it's very much science, as good science as we're capable of.
Feel free to provide a nicer model that still explains the current observations, though. I'm sure the Nobel Foundation will reward you for your efforts if you get it right enough!