When the neutron:proton ratio is 1:1
It is for this reason that large nuclei contain proportionally more neutrons than light elements
They form heavier elements
Nuclear fission: When an element breaks apart to form lighter elements and other sub-atomic particles. Nuclear fusion: When two lighter elements fuse to form heavier ones.
Good question. A fusion bomb combines (fuses) light nuclei (hydrogen) into larger nuclei to get its energy. But it needs a fission bomb to start it. A fission bomb breaks up (fissions) heavy nuclei (uranium/plutonium) into smaller nuclei to get its energy.
No, citric acid is stable in normal light.
It is for this reason that large nuclei contain proportionally more neutrons than light elements
No. Fusion is the combining of light elements into heavier elements (like 2 deuterium into 1 helium). radioactive decay is when you have an unstable atom releasing energy (and sometimes matter) in order to reach a more stable state.
They form heavier elements
Stars obtain energy through the majority of their lives by the process of thermonuclear fusion of the nuclei of light elements to produce nuclei of heavier elements. Initially the processes fuses hydrogen nuclei, producing helium nuclei (similar to what hydrogen bombs do), but the process ceases when it produces nickel and iron nuclei at which point the star begins dying as it has run out of nuclear fuel.
The two elements are elements 43, Tc, technetium, and 61, Pm, promethium. Technetium has a few "nearly stable" isotopes with half-lives of over a million years. Promethium's longest lived isotope has a half-life of about 20 years.
light
fusion
No. Alpha particles are helium nuclei; such nuclei have a mass, and can therefore NOT travel at the speed of light.
The formation of the elements is a nuclear process that usually happens in stars. The core of the star is hot enough and has enough pressure to overcome the electric repulsion of the atomic nuclei and literally fuse the nuclei together. This process happens over and over again, but seems to stop at a certain mass. It appears that elements heavier than iron cannot be formed in the core of a star. These elements require more extreme conditions. The heavier elements on the Periodic Table (after Fe) are formed in supernova. These nuclei require tremendous energy to form, this energy must come from an event as large as a supernova.
fusion
Albert Einstein
The combination of two light atomic nuclei to form a heavier nucleus is called fusion.