149 points by lainon 7 days ago
This is really brilliant, literally jaw-dropping. I was really blown away by the idea and construction of the detector itself and this application is astounding.
My favourite story about the construction of IceCube relates to the drilling of the holes to deploy the detector. They used two types of drill, which melt the firn (compacted snow) on top and ice lower down. One is a sort of conical heat exchanger, the other circulates water through a Big water heater on the surface.
In the early days of South Pole Station (late 1950s), supplies were airdropped in - the cargo planes of that era couldn't land on the snow and going overland was very difficult. Many of the parachutes wouldn't open properly, and so lots of supplies (including a bulldozer) and parachutes wound up buried in the snow. South Pole slowly accumulates snow, so that debris has gotten deeper and deeper below the surface over time.
Of course, the holes required to build IceCube had to go deeper than those supplies, but the drill can't go through things that don't melt, so in some cases the holes had to be moved off the nominal grid. According to the story I heard, one of the holes ran in to a bunch of meat, which floated to the top of the bore...
No mentions about finding meat here, but you might be interested in this story at IEEE Spectrum about the construction of IceCube from 2011 .
You may like KM3NeT then (http://www.km3net.org/). The goal is to build a cubic kilometer spanning instrument at the bottom of the Mediterranean.
Wikipedia has a good artist's conception picture of it:
Agreed. This is truly astounding. Neutrinos seem to encapsulate an unnaturally high degree of complexity and information in such a tiny package ;)
Formalism of Neutrino Oscillations
I always thought that if an alien civilization is trying to communicate with earth, they would do it via neutrinos and not radio waves, because if you know where you are communicating to, you don't need to worry about signal attenuation as much as with EM waves.
Supplementary Figure 6 is pretty cool! There seems to be a lot of strange things happening at the mantle-crust boundary that will take some further study to understand.
All said, this is a MAJOR advance in our understanding of the Earth and the science thereof. This technique should allow for some pretty amazing things in the future.
Would it be feasible to put a source and detector in orbit so we could get high resolution CT images of the interior of the earth? IIRC the detector used here is very large, but there are smaller ones and a directed source would go a long way towards making the detection simpler.
Neutrino detection generally requires large volumes and large masses (for very large values of "large"), neither of which are as yet feasible for space based systems. The IceCube neutrino observatory, for example, makes use of a volume of ice that is on the order of a cubic kilometer (over 900 million tonnes). Suffice it to say, building cubic kilometer solid structures in space that weigh hundreds of millions of tonnes is outside of our engineering capabilities at present. However, within the next several decades this might be feasible.
That's also understating the size. While the final detection is happening in the ice, the column of air above it is also important.
Could we not just land a detector on the far side of the moon. Thats pretty large no?
It is but you need both a big hunk of mass and a way to detect the neutrino interactions inside it. Ice Cube is shot through with detectors. One of the OG detectors measured the particular isotope created during interactions.
The Super-Kamiokande has photomultipliers staring at a bunch of water looking for Cherenkov radiation resulting from neutrino interactions
None of these are much of a practical option with the moon.
You need to have the reaction mass to make use of. Most neutrino detectors use special chemicals in custom tanks, IceCube uses antarctic ice. You would need not just mass but ice or water for a neutrino detector, ideally highly compressed optically clear ice. The only possible candidate in the Solar System that fits that bill at present is Europa. Though it's possible that similar conditions might also exist on Mars (we know there are sub-surface glaciers, but we don't know how deep they go or how pure the ice is. And potentially some of the large sub-surface oceans (on Ganymede, Enceladus, etc.) might work too but we know even less about their properties.
Not all detectors were optical so if you found a moon made of, say, dry cleaning fluid, you'd still be good.
Each detector has a limited range. And only works well in certain mediums, generally water or water ice. Even if the Moon was solid ice, we would need to surround it with detectors, as well as drill a huge number of holes all the way through it and place detectors (probably hundreds of thousands or millions) in each hole.
I had this idea back in my undergrad when my professor first told me about neutrinos (which was his forte). The harder I looked the more infeasible it seemed. The big problem, is creating a detector. The reason this is a big problem is because neutrinos are so small and so neutral. How small? An electron is 511keV. A neutrino is <= 0.21eV. That's 7 orders of magnitude! And on top of that, they have a neutral charge. There is no electric dipole moment either. So how does it interact? Basically by striking another particle. And remember that atoms are basically empty space. So chances of that are slim.
So to place a detector in orbit we'd need one of two things. Space travel to become cheap enough where putting a massive body up is cost feasible, or a radically different understanding of how to detect neutrinos. (First is more likely)
The former also comes with some problems. You'll find more about this by asking why detectors are so far underground. And there's a big connection there to generating the resolution you'd need to map the interior of the Earth.
An in space detector is (at least to my understanding) not that easy, as you need the surface of the Earth to interact with the neutrinos. These interactions result in muons, which allow to detect that there was a neutrino in the first place. Also, there is a pretty big source for neutrinos pretty close to Earth, but Earth is in its orbit, as opposed to the other way around.
The IceCube neutrino detector consists of about a cubic kilometer of ice. You're not going to put one of those in orbit.
But it would make a cool joint project for NASA and the NSF to fund. Capture a comet big enough that you could mine enough water to make a cubic kilometer sized detector in Earth orbit.
That could probably also wipe out half a continent if you mis-aim it...
Then again, it would look spectacular in the sky!
There are other types of neutrino detectors. Not that it really makes the problem any easier to solve, but this isn't the only way.
That's what I was thinking. They have sent neutrinos from one lab to another with a man-made source and a detector smaller than 1km^3. The idea is to put a strong source in orbit and aim it at an orbiting detector. Over time this configuration would be used to scan the entire planet. Still a huge challenge.
That's essentially the main idea most people come to. Using a source so you can concentrate on specific ones and not get distracted by solar, cosmic, or terrestrial neutrinos. Or you could just use terrestrial ones. But still, that detector is the hardest part to figure out.
You might be able to tow it in from elsewhere using a light sail, however. Beyond our current technology, but might be doable by 2100, or sooner with a fortuitous comet trajectory.
And once it is in orbit, how do you propose stationkeeping against exospheric drag? Preferably a solution that will remain reliable for 10^n (n>>3) years.
A cubic kilometer of ice is 9.167e11 kg.
Also, just keep the orbit above 800km, and the light sail will still be able to counteract its own drag.
If the orbit gets too low, turn the ice into rocket fuel and use it to refuel ships boosting into higher orbits.
I'm pretty sure that a cubic kilometer of ice in orbit would have more value in other purposes than as a neutrino detector!
Sure, but as long as it's up there, might as well use it in every way possible.
The muons are produced in the upper atmosphere (from cosmic rays interacting with the atmosphere). You can't do this in space. Not too mention the size of a neutrino detector, although you can use the e.g. regolith of the moon as a neutrino detector (via the Askaryan effect). In fact there are experiments pointing radio telescopes at the moon to look for ultra-high-energy neutrino interactions. My not-so-polite term for them is lunatics :).
Oh you :)
Nice but I'm still left wondering what the J/bit of neutrino transmission would be. Wouldn't it be cool if we could replace the long fiber optics stretching around the globe with direct-through neutrino stations?
Given the difficulty in neutrino detection, I seriously doubt it would replace fat links. You could gain quite a bit of advantage when it comes to trading though using a low bandwidth link.
https://what-if.xkcd.com/73/ gives a fairly decent summary of the level of interaction of neutrinos.
Frankly this idea has been repeated every few years since the invention of tomography 40 years ago. Hopefully someone will actually do it one of these years.
In theory, would IceCube be able to detect neutrinos generated by the same mechanism in the atmosphere of Venus?
In theory, yes. In practice, probably very difficult. They did detect a deficit in neutrinos from the direction of the moon though .
Could this technique be useful on other planets?
Looks like my prediction will come true.
> Neutrino detection will revolutionize oil and other natural resource discovery.
To be fair, it probably will. But the ability to do it in a cheap enough manner is certainly far enough away that the value of those resources will likely be much lower than they are today.
Accurate, cheap, and small neutrino detectors would revolutionize any industry dependent upon locating things within... well... anything. But that statement is as meaningful (if not less) as "faster computers will revolutionize the automotive industry."