This is a picture of our sun -- not remarkable, you might think. Pretty grainy and crappy actually. The cool part is... it was taken at night.
Normally of course you can't see the sun at night because the Earth gets in the way. This was taken looking through the middle of the Earth. Like if you pointed a camera straight down at the ground at midnight, and saw the sun on the other side.
How the hell did we do this? Well the picture isn't taken using light (photons). It's taken using amazing little particles called neutrinos.
The amazing thing about neutrinos is that they're ghostly and virtually invisible. Zillions of them zoom through us every second without leaving a trace! And they can pass straight through the Earth just as easily. Ordinary light (photons) can be stopped by just a thin sheet of paper, and a thin sheet of lead will stop even high-energy gamma-ray photons, but it would take a few light-years of lead to stop an average neutrino from the sun. To put it another way, if you filled the whole distance from the Earth to the sun with solid lead, 99.999% of the neutrinos would pass through unaffected!
You might wonder, if they're so ghostly, how do we see any at all? Mainly there are just so many zillions of them coming from the sun that with a big enough and sensitive enough detector we can see a few. So physicists have built gigantic detectors made out of huge vats of liquid, and buried them deep inside the Earth where nothing can reach them except for neutrinos. For example, the Super-Kamiokande detector is inside a mountain in Japan (Mt Ikenoyama, Gifa prefecture) and contains 20 Olympic-sized swimming pools worth of water. That's where the picture above was taken. It took a year and a half. (!)
One of the cool experimental developments in particle physics & astrophysics today is the development of actual neutrino telescopes! These are designed to not just see neutrinos, but to look at far away objects using them! There's numerous uses for this. Since neutrinos are so ghostly, neutrino telescopes offer a sort of 'X-ray vision' -- they can see inside things like neutron stars, supernovae, and GRBs and help us better understand how they work. And by observing neutrino cosmic rays, they will be able to test some new theories of physics. They may even be able to detect dark matter.
(Indeed neutrinos are a perfect example of dark matter themselves! We feel their gravitational interaction, but they're so weakly interacting they're hard to see any other way. For a while people thought the dark matter might actually be just neutrinos. But recently we've accumulated evidence that shows neutrinos make up only a small fraction of the missing dark matter -- most of it has to be something else.)
More info:
PBS: The Ghost Particle:
http://www.pbs.org/wgbh/nova/neutrino/http://en.wikipedia.org/wiki/Neutrinohttp://hyperphysics.phy-astr.gsu.edu.../neutrino.html
http://www.physics.ubc.ca/~waltham/sno_talks/tno.pdfICECUBE:
http://icecube.wisc.edu/Super-Kamiokande:
http://neutrino.phys.washington.edu/~superk/http://www.newscientist.com/channel/...mg18524885.900source: bluelight forums, posted by Zorn, a phys grad student
http://www.bluelight.ru/vb/showthread.php?t=274174