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GCSE level Physics notes on Cosmology: Part 4.
In cosmological terms what is the red-shift? The role of redshift in cosmology - evidence for
a big bang model
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INDEX for physics notes on
COSMOLOGY
(4)
In cosmological terms what is the red-shift?
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You should have read Parts 2
and 3 before studying Part (4)
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(2)
Explaining the Doppler effect in a
cosmological context
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(3)
Why do we get light from stars? How do we
analyse this light?
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What is the red shift phenomena?
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The light from distant galaxies seems
to be of lower frequency than expected.
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Hydrogen gives a series of
specific spectral lines eg one in the red, one in the green, several in the
blue and many in the indigo and violet region (which are not numbered in the
diagram below).
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The vertical black lines
in the diagram below represent the visible light frequencies absorbed.
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Now, if we bring in the idea of the
Doppler effect, we can use this stellar (stars, galaxy, nebulae) absorption spectrum as
evidence to show that the universe is expanding.
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So instead of racing cars or
trains, think stars, if the galaxies are moving away from us, then the light
waves will be stretched out over the billions of miles so that the
wavelengths get longer - which is in the red direction of the visible
spectrum!
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When the spectra from galaxies from a
variety of huge distances away from Earth, a pattern was noticed, first recognised by
American astronomer Walter S. Adams in 1908.
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The pattern of spectrum of
lines of elements like hydrogen seemed to be the same, BUT, the
frequencies were smaller, wavelengths longer, than what you observe on
Earth e.g. from the Sun, our nearest star.
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The shift to lower frequencies called the
red-shift because
the 'shift' was towards the lower frequency red end of the visible
spectrum.
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It is an example of the Doppler Shift described in section 1.
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The astronomer Edwin Hubble in 1929,
recognised the spectral pattern for hydrogen, but realised all the
wavelengths were shifter to longer values.
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He
further analysed the red shifts and related the increasing value of the
shift to faster more distant galaxies appearing to move away from us at
great speed.
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The red-shift to longer
wavelengths and lower frequencies is indicated by the white arrows on the diagram
below.
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I've only indicated the shift
for the first two lines in the spectrum of hydrogen (a fragment of the
spectral patter for hydrogen, but enough to illustrate the red shift).
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1. goes deeper red and 2. goes from
green to yellow-green to yellow (still described as a 'red shift').
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Notice that the 'pattern of lines', the
hydrogen spectral 'fingerprint' remains the same.
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Also note that
the more distant the
galaxy, the greater the red shift in frequencies/wavelengths.
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The vertical black lines represent the emission or
absorption spectrum of hydrogen.
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The indigo should a dark blue and
violet,
but on saving the graphic image, a few curious effects happened, sorry about
that, but it doesn't detract from the explanation of the 'red shift'!
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As you can see from the diagram, the more
distant the galaxy, the bigger the red shift - the more the waves are
stretched out with a longer wavelength and lower frequency.
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==>
==>
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The spectral lines observed from Earth of: our Sun
==> distant galaxy ==> very distant galaxy, and this change,
the 'red shift' in wavelengths and frequencies applies to the whole
pattern of spectral lines of any element, but is best observed, and
first discovered, by studying the light from very hot hydrogen atoms.
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What Hubble and other astronomers found
that the further a galaxy is from us (the observer) the faster the
galaxy seems to moving away from as.
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These speeds are calculated from the red-shift.
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Cosmologists have therefore concluded
that the whole of the universe is expanding (See Part (5).
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INDEX for physics notes on
COSMOLOGY
Key points for Physics - The Red-Shift effect in
cosmology
Information
sources for Doc Brown's key points: IGCSE-GCSE physics are based on textbooks
& syllabus-specifications for students taking the UK AQA,
Edexcel, OCR 21st Century Science, OCR Gateway science suite, WJEC, CCEA &
CIE GCSE
physics 9-1 level science examinations.
A clear and exam-board-friendly set
of summary revision notes on cosmological red-shift,
tailored for WJEC, CCEA, CIE, AQA, Edexcel, and OCR
GCSE/IGCSE Physics students:
Cosmological Red-Shift – GCSE/IGCSE
Physics Revision
What Is the Red-Shift?
- Red-shift
is the increase in the wavelength of light from a
source moving away from the observer.
- In cosmology, it refers to the
stretching of light waves from distant galaxies, shifting them
toward the red end of the visible spectrum.
- This is a result of the
Doppler effect applied to light.
What Does It Tell Us?
- Distant galaxies show red-shifted
light, meaning they are receding from us.
- The greater the red-shift,
the faster the galaxy is moving away.
- This provides strong evidence that the
Universe is expanding.
Supporting the Big Bang Theory
- Red-shift supports the Big
Bang Theory, which proposes the Universe began from a hot,
dense state and has been expanding ever since.
- Hubble’s Law:
The speed at which a galaxy moves away is proportional to its
distance from Earth.
Student Tips
- Use diagrams
to show red-shift and wave stretching.
- Remember: Red = Receding.
- Practice explaining how red-shift
supports the expanding universe.
- Know the difference
between red-shift and blueshift.
- Use past paper questions
to get used to phrasing like “how does red-shift support the Big Bang?”
Keywords, phrases and learning objectives for
the red-shift
In cosmology know what is meant by the red-shift
(e.g. in the spectral lines of hydrogen).
Know how and why the spectral lines of hydrogen
light from distant stars galaxies are shifted to longer wavelengths
and lower frequencies by the Doppler effect.
Appreciate how the observed red-shift provides
evidence that the universe is expanding and supports the ‘Big Bang’
theory (that the universe began from a very small initial point),
rather than the 'steady state' theory.
Explaining the importance of explaining
the red shift as evidence of universe expansion
in GCSE level physics, What you need to know about explaining the red
shift as evidence of universe expansion for
GCSE level
physics,
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