Birth of a star
I can describe what a star is and how it forms.
Birth of a star
I can describe what a star is and how it forms.
These resources will be removed by end of Summer Term 2025.
Lesson details
Key learning points
- The Sun is a medium sized star that emits radiation as a result of nuclear fusion reactions in its core.
- A star is formed from a cloud (nebula) of dust and gas pulled together by gravitational attraction.
- Dust in a nebula is any sort of fine particle, such as specks of rock, and most of the gas in space is hydrogen.
- As a star forms, dust and gas accelerate towards its centre over a very long time, creating very high temperatures.
- A star forms when hydrogen nuclei in a protostar fuse together converting mass into gamma radiation that causes heating.
Keywords
Star - a ball of very hot gas and plasma that emits radiation and is powered by nuclear fusion in its core
Nuclear fusion - the process of merging small nuclei into larger nuclei with the release of energy
Nebula - a region of space containing traces of gas (mostly hydrogen) and dust
Protostar - a dense, hot, ball of gas formed by a collapsed nebula
Main sequence star - the stable period of a star when it is fusing hydrogen in its core
Common misconception
The Sun is not a star.
Compare the properties of the Sun with those of stars to show they are similar.
Licence
This content is © Oak National Academy Limited (2024), licensed on Open Government Licence version 3.0 except where otherwise stated. See Oak's terms & conditions (Collection 2).
Lesson video
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Starter quiz
6 Questions
a large spherical object that orbits a star
a very hot ball of gas and plasma that emits light radiation
a group of billions of stars clustered together in space
the whole of space and everything in it