Unit 6: Sound and space
Nebulae — HIA International - Grade 8 Revision Notes & Topical Questions
5 min read 8 parts Lesson 11 of 14 1 quiz
Lesson summary
Nebulae — HIA INTERNATIONAL notes: Describe nebulae, their composition and how stars form in stellar nurseries.Nebula = a cloud of dust and gas in space; the plural is nebulae.Gases — mostly hydrogen with a smaller quantity of helium.Density — the particles are very far apart; a …
- Compared with a galaxy
- From dying stars
- Northern hemisphere
- Southern hemisphere
- Stellar nursery
- Not all nebulae
Section 1 of 8What a nebula is
Nebula
Nebula a cloud of dust and gas in space; the plural is nebulae.
Gases
- Gases mostly hydrogen with a smaller quantity of helium.
Density
- Density the particles are very far apart;
- a nebula the size of the Earth would have a mass of only a few kilograms.
Size
- Size most are very large, many more than 10 000 times bigger than the Solar System.
Compared with a galaxy
- Compared with a galaxy a nebula is a cloud in space and a galaxy is a huge collection of stars.
Section 2 of 8How nebulae form
From dying stars
- From dying stars some form when giant stars reach the end of their life and explode, sending dust and gas over a wide area.
Recycling
- Recycling material from dead stars, including carbon, oxygen and iron, is recycled into new nebulae, stars and planets.
Glow
- Glow hot stars nearby heat the gas or light the dust; dark nebulae block light from stars behind them.
Section 3 of 8Examples
Northern hemisphere
- Northern hemisphere the Orion nebula is easy to see without a telescope.
Southern hemisphere
- Southern hemisphere the Tarantula nebula is visible without a telescope.
Hemisphere
Hemisphere half of the Earth, north or south of the equator.
Size
- Size the Orion nebula is 24 light years across.
Section 4 of 8Stellar nurseries
Stellar nursery
Stellar nursery an area in space where stars are formed.
Not all nebulae
- Not all nebulae only some types of nebulae act as stellar nurseries.
Young stars
- Young stars some are only half the mass of the Sun and have not yet reached full brightness.
Section 5 of 8How a star forms
1
Gravity pulls dust and gas together.
2
As the mass collects, the inward pull of gravity increases.
3
The pressure inside the new star becomes very large.
4
The high pressure causes heat.
5
Atoms react with each other (nuclear fusion), so the star gives out heat and light.
How a star forms
Planets
- Planets leftover material spinning around the star forms a flat disc that clumps into planets, moons, asteroids and comets.
Our Solar System
- Our Solar System formed in this way about 4.6 billion years ago.
Section 6 of 8Observing nebulae
Telescopes
- Telescopes the Hubble Space Telescope takes photographs of nebulae from space.
Infrared
- Infrared telescopes that detect infrared, such as James Webb, can see through dust to stars forming inside nebulae.
Section 7 of 8Key terms
| Term | Meaning |
|---|---|
| Nebula | A cloud of dust and gas in space. |
| Stellar nursery | An area in space where stars are formed. |
| Hemisphere | Half of the Earth, north or south of the equator. |
| Gravity | The force that pulls dust and gas together. |
| Nuclear fusion | Atoms reacting in a star to give out heat and light. |
| Light year | A unit of distance used in space. |
Section 8 of 8Exam technique
1
A nebula is the same as a galaxy — a nebula is a cloud of dust and gas; a galaxy contains many stars.
2
Nebulae are dense — their particles are very far apart.
3
All nebulae make stars — only some act as stellar nurseries.
4
Nebulae are made mainly of oxygen — they are mostly hydrogen and helium.
Marked practiceQuizzes for this lesson
Last updated: