BBC Home

Explore the BBC

h2g2
26th December 2009
Accessibility help
Text only

Guide ID: A623279 (Edited)

Edited Guide Entry


SEARCH h2g2
Edited Entries only
Search h2g2Advanced Search


New visitors: Create your membership
Returning members: Sign in
BBC Homepage
The Guide to Life, The Universe and Everything.

2. The Universe / Space, Stars and Galaxies

Created: 29th August 2001
Doppler Effect in Reference to Stars
Contact Us


Like this page?
Send it to a friend!

 

'The Universe is expanding'. You have probably heard that said many times. It may sound unbelievable but it is true. This has been proven by scientists looking at the Doppler Effect, otherwise known as the Red Shift Effect, and Fraunhofer Lines.

Fraunhofer Lines

All stars, including the Sun, emit electromagnetic (EM) radiation at many different wavelengths; only some of these are visible to the human eye. If you were to shine light through a prism you would see the spectrum of colours. This was first done by the great English mathematician, Sir Isaac Newton (1642 - 1727); although he did not follow up the discovery of the spectrum with any further research.

The different colours seen are different wavelengths of visible light. In 1802, the English chemist William Hyde Wollaston (1766-1828) discovered that the solar spectrum was not uniform. It contained dark lines at certain wavelengths. He mistook these lines as the boundaries between colours. We now know that the colours are continuous.

It was not until 1814 that German optician, Josef Fraunhofer (1787-1826), studied these lines in greater detail. He noted the positions of 324 them; although he still couldn't explain them.

Finally, in 1859, two more Germans, Gustav Kirchhoff (1824-1887) and Robert Bunsen1 (1811-1899), invented an instrument for separating light using prisms, which we know as the Bunsen-Kirchhoff spectroscope; founded the modern science of spectroscopy; and discovered the true reason for what were by then called Fraunhofer Lines. They found that certain elements absorb some wavelengths, which means that the elements found in the sun create black lines in the spectrum.

Doppler Effect

When an object is moving, any waves it emits are either stretched or squashed, so the wavelength either increases or decreases. In sound this makes something moving towards you sound higher, and something moving away sound lower. In light, an object such as a star, will be shifted towards the red end of the spectrum when moving away from you and towards the blue (or violet) end when coming towards you. The faster the object is moving, the greater the shift.

How This Proves Expansion Theory

Scientists knew that if the universe was expanding, then space would be stretched. This meant that anything in the space would also be stretched. This stretching is too small to be noticed in matter because gravity counteracts it; but in EM waves this is noticeable as a red shift.

When this red shift in the Fraunhofer lines of distant stars and galaxies was noticed it was clear proof that both the Expansion and Big Bang theories were correct. All other theories, such as Steady-State Theory2, were generally disregarded.

Another useful consequence of this is that the further away an object is, the more space the light has travelled through so it will be more red shifted, this allows astronomers to accurately calculate the distance of other galaxies.

Other Entries in this Project


1 Robert Bunsen was the inventor of the most familiar piece of equipment in the chemistry lab, the bunsen burner.
2 The Steady-State Theory describes a uniform, infinite universe that is basically the same everywhere. Opponents of this theory argue that it fails to account for differences in background radiation or for some parts simply being more fashionable than others.


Clip/Bookmark this page
This article has not been bookmarked.
ENTRY DATA
Written and Researched by:

Tango

Edited by:

John the gardener says, "Free Tibet!"

Referenced Entries:

Web-safe Colours
What's the Point of Astronomy?
The Sun
Stars
Travelling to the Stars
Betelgeuse - the Star
Astronomical Distance Scales
The Celestial Sphere
The Hubble Space Telescope
Universal Red Shift
The Big Bang
Blue - the Pigment of the Chemist's Imagination
The History of Optical Science



CONVERSATION TOPICS FOR THIS ENTRY:

Start a new conversation

People have been talking about this Guide Entry. Here are the most recent Conversations:

TITLE
LATEST POST
misleadingMay 19, 2005
Red shiftApr 21, 2005
ApproachFeb 12, 2002




Disclaimer

Most of the content on h2g2 is created by h2g2's Researchers, who are members of the public. The views expressed are theirs and unless specifically stated are not those of the BBC. The BBC is not responsible for the content of any external sites referenced. In the event that you consider anything on this page to be in breach of the site's House Rules, please click here. For any other comments, please start a Conversation above.




About the BBC | Help | Terms of Use | Privacy & Cookies Policy