Skip to main content

About this free course

Download this course

Share this free course

In the night sky: Orion
In the night sky: Orion

Start this free course now. Just create an account and sign in. Enrol and complete the course for a free statement of participation or digital badge if available.

Tuesday, 5 Jul 2022, 17:48
Site: Open Learning
Course: In the night sky: Orion (INS_1)
Glossary: Orion Glossary

near Earth asteroid

An asteroid that has an orbit that brings it close to the orbit of the Earth (defined as any asteroid that comes within 1.3 astronomical units from the Sun). Abbreviated to NEA.

neon burning

The process by which massive stars fuse a neon and helium nucleus together to produce a magnesium nucleus, releaseing energy in the process.

neutron star

When a high-mass star runs out of nuclear fuel, it will undergo a type II supernova explosion and its core will collapse to form a neutron star. A neutron star has a mass similar to that of the Sun, but a radius of only about 10 km. A neutron star is supported against gravity by an effect of quantum physics known as neutron degeneracy pressure. See also white dwarf, black hole.

nuclear fusion

The fusing together of two atomic nuclei to make a larger nucleus. There is a decrease in the total mass of the nuclei in a fusion reaction, so this process results in the release of large amounts of energy, according to Einstein’s equation E = mc2.

nuclear reactions

Processes in which two or more nuclei are involved, resulting the creation of different nuclei from those originally present. See also nuclear fusion.


The process by which the nuclei of elements (other than hydrogen) are formed. There are believed to be three sites (or epochs) where (or when) nucleosynthesis occurs (or has occurred). Light nuclei, such as deuterium, helium and lithium, were formed in the early Universe when the Universe was between about 100 s and 1000 s old. Nuclear fusion inside the cores of stars is responsible for the formation of more helium nuclei, and also for the formation of other nuclei up to those with a mass around that of iron. Supernovae explosions are responsible for the formation of more massive nuclei.