Each helium nucleus has two protons and two neutrons.
Under very hot temperatures — greater than 100,000,000 Kelvin (179,999,540.6 F) — the helium nuclei begin to fuse, first as pairs into unstable 4-proton beryllium nuclei, and eventually, as enough beryllium nuclei blink into existence, into a beryllium plus a helium.
Carbon is also the key ingredient for most life on Earth; the pigment that made the first tattoos; and the basis for technological marvels such as graphene, which is a material stronger than steel and more flexible than rubber.
The basis for the carbon 14 dating method is that Flash german imagechat
The end result: Atoms with six protons and six neutrons — carbon.
While scientists sometimes conceptualize electrons spinning around an atom's nucleus in a defined shell, they actually fly around the nucleus at various distances; this view of the carbon atom can be seen here in two electron cloud figures (bottom), showing the electrons in a single blob (the so-called s-orbital) and in a two-lobed blob or cloud (the p-orbital). It can link to itself, forming long, resilient chains called polymers.
The primary source of carbon in today's world is the deposits of coal that are mined.
There are 3 allotropes of carbon that are found naturally - graphite, diamonds, and amorphous carbon.
A radioactive isotope of carbon, known as carbon-14, is used for the purpose of carrying out this activity.