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CIE 0625 Physics · IGCSE · Topic 6.2

Stars and the Universe

Clear, syllabus-mapped CIE 0625 Physics revision notes on stars and the universe: explanations, worked examples and exam technique, then a free targeted practice drill.

CIE 0625 PhysicsIGCSEFree revision notes
Contents: 7 sections

Cambridge IGCSE Physics 0625 · Core and Extended

Syllabus points

Stars

A star is a body that emits its own light, powered by nuclear fusion. In the core, hydrogen nuclei fuse to form helium, releasing energy.

The Sun is an ordinary star, unremarkable except for being close. It appears far brighter and larger than other stars for that reason alone.

A star is stable while two effects balance: gravity pulling it inwards and the outward pressure produced by the energy released in fusion. The whole life cycle is the story of that balance holding and then failing.

Galaxies and distances

A galaxy is a huge collection of stars, held together by gravity. Our galaxy is the Milky Way, and the Solar System is one of many systems within it.

The Universe contains billions of galaxies, separated by vast distances.

The light-year

A light-year is the distance light travels in one year. It is a unit of distance, not of time, and calling it a length of time is the standard error.

light-year = speed of light x time in one year = 3.0 x 10⁸ x (365 x 24 x 60 x 60) = about 9.5 x 10¹⁵ m

The nearest star beyond the Sun is about 4 light-years away, and the Milky Way is about 100 000 light-years across.

Because light takes time to arrive, looking at distant objects is looking into the past. Light from a galaxy a million light-years away left it a million years ago.

The life cycle of a star

A star begins as an interstellar cloud of gas and dust, mostly hydrogen. Gravity pulls it together, and it heats as it contracts. When it is hot enough for fusion to begin, a protostar becomes a stable star.

The star spends most of its life in this stable phase, which for the Sun is about ten billion years.

When the hydrogen in the core runs low, the balance fails and the star swells:

For a star about the size of the Sun:

  1. Stable star
  2. Red giant as the outer layers expand and cool
  3. White dwarf as the outer layers drift away and the hot core is left
  4. It cools slowly and fades

For a star much more massive than the Sun:

  1. Stable star
  2. Red supergiant
  3. Supernova, an enormous explosion
  4. The remnant becomes a neutron star, or a black hole if the star was massive enough

The route taken depends on the star's mass, and questions ask which path a given star follows.

Elements heavier than iron are formed in supernovae and scattered into space. The material of the Earth, and of us, was made in earlier generations of stars.

Redshift

Light from distant galaxies is shifted towards the red, or longer-wavelength, end of the spectrum. This is redshift, and it indicates that the galaxy is moving away from us.

The key observation is that the further away a galaxy is, the greater its redshift, and so the faster it is receding.

This is the evidence that the Universe is expanding. It does not mean the Earth is at the centre of that expansion: an observer in any galaxy would see the same thing, because space itself is expanding and every galaxy is moving away from every other.

The Big Bang

Running the expansion backwards suggests the Universe began from a single point, expanding from an extremely hot, dense state. This is the Big Bang theory, and the estimated age of the Universe is about 13.8 billion years.

Two pieces of evidence support it:

The CMBR is the more decisive of the two, because the Big Bang predicted it before it was found.

Common mistakes

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