An unstable nucleus becomes more stable by emitting radiation. Alpha decay throws out a helium nucleus, beta decay throws out an electron (β−) or a positron (β+) as a neutron and proton swap, and gamma emission releases a high-energy photon. In every nuclear equation the mass numbers and the atomic numbers each balance on both sides, so the emission tells you exactly which element is left behind. This is the real knowscape from knowhere, not a picture of one. Drag it. Watch what actually changes.
Every nucleus here is chasing a tighter grip. Unstable ones throw out alpha, beta or gamma, heavy ones split, light ones fuse, and each step ends more tightly bound and slightly lighter. That missing mass is the energy, via E=mc², whether it runs a reactor or hits your cells.
A nucleus fires an alpha particle, a beta-minus electron, a beta-plus positron or a gamma photon at paper, aluminium and lead. The nuclear equation above it fills in the daughter element as the mass and atomic numbers balance, and each emission stops where its penetrating power runs out.
knowhere maps every concept to what it rests on and what rests on it — 3 underneath this one, 2 built on top. Each one says why, in a sentence, not as an arrow on a diagram.
Each one is its own knowscape in the app — built for how a particular student takes things in, not one explanation handed to everybody.
Every HSC and VCE concept in knowhere is built like this one — mapped to your curriculum, never capped by it. Free for a week. No lock-in, cancel inside the week and pay nothing.
Free for a week, then a plan you can stop any time.
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