That confused me for a moment so it seems worth clarifying: in ice, certain particles can travel faster than light does in ice.
I assume this is not a hard, totalizing law since it seems we're able to get samples of neutrino collisions in just a kilometer sized chunk of ice on Earth (meaning that the probability of collision is not absolutely zero and there's no way to know the full neutrino travelogue through the universe)
to put things to scale 1 ly is 9,460,730,472,580,800 meters, or 63,241.077 astronomical units, the distance from the Earth to the Sun.
Needless to say, it's pretty weakly interacting as far as interaction goes...
Identifying the origin let us see objects behind dust clouds or other obstacles.
How does this not violate conservation of momentum? Are you saying every single collision is head-on?
In other cases, the particle being collided is scattered and won't show up in the detector. Low energy neutrino collisions also have very faint light and difficult to detect. Solar system produced neutrinos are in this category.
- In the beginning, for the first couple of events, only because they have way higher energies than anything in the solar system could produce - By now, with enough data collected, their origin correlates very well with the milky way - we are close to identifying several far away galaxies as well
This is the significance. Contrary to some statements published today, IceCube was not primarily built to study Neutrinos, it was built to study the universe using Neutrinos.
That's why we care where they are coming from, we want to learn about the astrophysical objects that produce them.
[1] https://www.amusingplanet.com/2015/07/the-surreal-world-of-n...
[2] https://news.cnrs.fr/videos/detecting-neutrinos-at-the-botto...