The Universe – WJECHubble’s law

The study of atomic absorption spectra allows us to determine the chemical make-up of stars. It shows that galaxies are moving away from us in an expanding Universe.

Part ofPhysics (Single Science)Forces, space and radioactivity

Hubble’s law

Edwin Hubble looked at the light from galaxies further away from Earth and realised that the dark absorption lines showed greater red shifts. He concluded that distant galaxies had bigger red shifts because they were moving away faster.

Five absorption spectra labelled: Very distant galaxy, Distant galaxy, Nearby galaxy, Nearby star and Laboratory reference.

The greater the distance from Earth, the bigger the red shift of the absorption lines.

Hubble used the red shift to calculate the velocities of galaxies against their distance from Earth.

When the data was put into a graph it showed a straight line through the origin.

A distance-velocity graph showing that the galaxies furthest away are moving away at a faster velocity than the galaxies closest to us.

This shows that the velocity of a galaxy is directly proportional to its distance away from Earth. In other words, if the distance of the galaxy away from us doubles, so does its .

This is Hubble’s law.

The Hubble constant (H) is the gradient of the graph. \(\frac{1}{\text{H}}\) gives us the age of the Universe – currently thought to be around 13.7 billion years.

As the recessional velocity increases with the distance of the galaxy, it implies that all the galaxies originated from a single point.