The nucleus is made of two kinds of particle, together called nucleons 核子:
- protons 质子, which have a relative 相对 charge of $+1$;
- neutrons 中子, which have a relative charge of $0$ (they are neutral).
An electron has a relative charge of $-1$. A proton and a neutron each have a relative mass of about $1$; an electron is almost massless in comparison.
Two numbers describe a nucleus:
- the proton number 质子数 $Z$ (also called the atomic number) — the number of protons;
- the nucleon number 核子数 $A$ (also called the mass number) — the number of protons plus neutrons.
So the number of neutrons is $A - Z$.
We write a nucleus in nuclide 核素 notation:
$$^{A}_{Z}\text{X}$$
where X is the chemical symbol. For example, $^{197}_{\ 79}\text{Au}$ has $79$ protons and $197 - 79 = 118$ neutrons. The relative charge of the whole nucleus is just $+Z$ (here $+79$), and its relative mass is about $A$.
Isotopes
Isotopes 同位素 are atoms of the same element (the same $Z$) but with different numbers of neutrons (different $A$). They behave the same in chemistry but differently in the nucleus. For example, $^{12}_{\ 6}\text{C}$ and $^{14}_{\ 6}\text{C}$ are both carbon.
Isotopes of carbon have the same six protons but different numbers of neutrons, so they are the same element with a different mass
Nuclear fission and fusion
In nuclear fission 核裂变, a heavy nucleus absorbs a neutron and then splits into two smaller nuclei, giving out two or three neutrons and a lot of energy 能量:
$$^{235}_{\ 92}\text{U} + ^{1}_{0}\text{n} \rightarrow\ ^{141}_{\ 56}\text{Ba} + ^{92}_{36}\text{Kr} + 3\,{}^{1}_{0}\text{n}$$
A neutron splits a U-235 nucleus into two smaller nuclei, releasing more neutrons and energy
The top numbers (nucleon numbers) balance on both sides, and so do the bottom numbers (proton numbers). You can use this to find a missing number — for example, how many neutrons are released.
In nuclear fusion 核聚变, two light nuclei join to make a heavier one, also giving out energy. This is how the Sun makes its energy, joining hydrogen 氢 nuclei to make helium 氦:
$$^{2}_{1}\text{H} + ^{3}_{1}\text{H} \rightarrow\ ^{4}_{2}\text{He} + ^{1}_{0}\text{n}$$
In fusion two light nuclei join into a heavier one, releasing a neutron and energy — the reaction that powers the Sun
In both fission and fusion, a small amount of mass is lost and turned into energy.
A nuclear power station uses the energy from fission to make electricity; the towers release waste heat as steam