Okay, so here I am again, home GMK. You may recall that back in October I promised to soon make a video on the radioactive triton. Well, it being February now, I think I start to renege on that promise, but at least it's finally here. Thank God for midterm break, say. So, the last video ended with the stable configuration of the Juiceron. Now, suppose a free neutron were to come close to one of these Juicerons. Naturally, since it doesn't have an electric charge, it would be very easy for the nuclear force to cause it to bind the Juiceron. This is what happens, and we get a triton. Now, you may recall what I said last time about a neutron being stable when it's bonded to a single proton, because otherwise the thing would fly apart. Well, in this case, two neutrons are really too much for just one proton, so this configuration is unstable. Me in lifetime is much longer though. For a free neutron, as you may recall, it was about 15 minutes. In this case, it's about 17 years. So, let's take a look at the decay now. It's beta-dk, so it emits a weak minus-poor sun, which decays into an electron anti-neufrino and an electron, and one of the down quarks transforms into an up quark. So, the whole thing becomes a helium, two protons and one neutron that is stable because of another neutron decays, and obviously the three protons will fly apart, so it has to stay that way. Anyway, it's a helium-3 nucleus distinct from an alpha-particle, which is a helium-4 nucleus. So, that's about it for this video. I'm not going to go on the record to say I'll definitely do anything else because it's probably not going to happen for a long time if I do. So, whatever I have an idea for, whatever I get time to do, I'll do.