9.3 cosmology

Cards (18)

  • The Doppler effect
    • The apparent change in wavelength of a wave as the source moves relative to an observer
    • Compression or spreading out of waves emitted or reflected by a moving source
    • Wavelengths in front are compressed and wavelengths behind are spread out
    • For a source moving away the wavelength increases
    • Red shift
    • For a source moving towards the wavelength decreases
    • Blue shift
  • Red shift
    • Evidence for expanding universe
    • All galaxies are red-shifting
    • The further away the galaxy the greater the red shift
    • Therefore the universe is expanding 
    • z=z=vc=\frac{v}{c}=Δff=\frac{\Delta f}{f}=Δλλ-\frac{\Delta\lambda}{\lambda}
    • v = objects receding velocity
    • The wavelength ratio is negative as the wavelength is inversely proportional to the frequency
    • Redshift z=z=vc  if  v<<c-\frac{v}{c}\ \ if\ \ v<<c
    • z is positive if moving away (red-shift) and negative for blue-shift
    • v is positive if moving towards
    • Ignores relativistic effects
    • Applied to optical and radio frequencies
  • Binary stars
    • Identified using the Doppler effect
    • Two stars orbiting a common centre of mass
    • Spectroscopic binaries = binary star systems where stars are too close to be resolved by a telescope
    • Only way to identify is by using the Doppler shift of each star
    • As the stars eclipse each other they are travelling perpendicular to the line of sight from the observer 
    • No Doppler shift in emitted radiation
    • When one star is travelling away from the observer the other is travelling towards
    • This causes each spectral line to split in two
    • One is blue-shifted and the other is red-shifted
    • Eclipsing binaries = when the plane of the orbit of the stars is in line of sight from Earth to the system
    • Stars cross in front of each other as they orbit
    • Can be identified from characteristic light curves
    Light curves
    1. No eclipse - brightness is maximum
    2. A larger star in front - blocks all light; the primary minimum
    3. No eclipse - brightness is maximum
    4. Smaller star in front - blocks some light; secondary minimum
  • Quasars
    • very large red shifts
    • Very far away
    • The power output must be around that of an entire galaxy
    • Proven with inverse square law
  • Hubble’s law
    • Spectra from galaxies all show a red shift
    • The amount of red shift gives the recessional velocity
    • The plot of recessional velocity against distance shows they are proportional
    • Suggests universe is expanding
    • v=v=HdHd
    • v = recessional velocity in kms-1
    • d = distance in Mpc
    • H = Hubble's constant in kms-1Mpc-1
    • Distance is difficult to measure so astronomers disagreed on the value of H
    • Ranging from 50 to 100
    • Now accepted H lies between 65 and 80
    • Most agree it is in the mid to low 70s
    • SI unit for H is s-1
    • Need v in ms-1 and d in m (1 Mpc = 3.08×1022m3.08\times10^{22}m)
  • Expansion of the universe
    • Cosmological principle = universe is homogenous and isotropic
    • Homogenous = every part is the same
    • Isotropic = everything looks the same in every direction
    • The universe doesn't have a centre
    • Until 1930s, cosmologists believed universe was infinite in space, time and static
    • The only way it could be stable using Newton’s law of gravitation 
    • Einstein modified the theory of general relativity to be consistent with the steady-state universe
    • Expanding and cooling down because it is a closed system
    • Must have been smaller and hotter
    • Evidence for Big Bang
  • Accelerating expansion
    • All the mass in the universe is attracted together by gravity
    • Slows down the rate of expansion
    • Thought the expansion was decelerating until 5 billion years ago
    • In the late 90s, astronomers found evidence that expansion is now accelerating
    • Explained using dark energy - a type of energy that fills the whole of space
  • Age of the universe
    • H=1t
    • If the universe has been expanding at the same rate
    • H=H=75kms1Mpc175kms^{-1}Mpc^{-1}
    • t=t=12.4×1018s =\frac{1}{2.4\times10^{-18}s}\ = 4.1×1017s  =\ 4.1\times10^{17}s\ \ = 13\ 13 billion years
    • Absolute size is unknown but there is a limit on the size of the observable universe
    • A sphere with a radius equal to the maximum distance that light can travel during its age
    • If H = 75, the sphere’s radius = 13 billion light years
    • Taking into account the expansion of the universe, the radius of the observable universe is thought to be 46-47 billion light years
  • Evidence for Big Bang
    • Assumed universe began from one point
    • A singularity infinitely small and hot
    • Suggests universe began with a huge explosion from this point
    • Thought there was high energy radiation everywhere
    • As the universe expanded and cooled radiation would lose energy and be red-shifted
    • CMBR = cosmological microwave background radiation
    • Remains of radiation
    • Microwave radiation detected from all directions in space
  • relative abundance
    • During the early stages of the Big Bang nuclear fusion converts hydrogen nuclei into helium nuclei
    • The universe cooled too much and fusion stopped
    • Approximately ¼ of all existing hydrogen nuclei were fused into helium
    • Relative abundance ratio H:He = 3:1
    • Relative abundance by mass of different elements 
    • 73% hydrogen
    • 25% helium
    • 2% everything else
  • Quasars
    • Discovered in the late 1950s and are thought to be stars in our galaxy
    • Spectra unlike normal stars
    • Sometimes shot out jets of material
    • Many were very active radio sources
    • Produced a continuous spectrum unlike the black body radiation curve
    • Had emission lines of elements unseen before instead of absorption
    • In 1963, Maarten Schmidt realised they were the blamer series of hydrogen but enormously red shifted
    • An active galactic nucleus 
    • Supermassive black hole surrounded by a disc of matter
    • As matter falls into the black hole jets of radiation are emitted from the poles
  • quasars
    • Characterised by:
    • Extremely large optical red-shifts
    • Very powerful light output
    • Their size is not much bigger than a star
    • Thought to be some of the most distant measurable objects 
    • Can estimate power output using inverse square law for intensity 
    • Use the amount of Doppler shift experienced by quasars to find their distance from earth
    • Shows quasars are extremely powerful and can have the same energy output as several galaxies
  • quasars
    • The first quasar to be discovered was 3C 273
    • Thought to be a dim star
    • Had much greater radio emissions than expected
    • Later found to be 26 billion light years away and 1000 times more luminous than the Milky Way
  • Exoplanets = planets that are not within our solar system
    • Orbit other stars
    • Can be difficult to detect directly
    • Tend to be obscured by the light of their host stars
  • Radial velocity method
    • Similar to detecting spectroscopic binaries
    • Star and planet orbit a common centre of mass 
    • Causes the star to wobble
    • Causes Doppler shift in the light received from the star
    • The effect most noticeable with high-mass planets
    • Have greater gravitational pull on the star
    • The line spectrum of the star is blue-shifted when it moves towards the Earth and red-shifted when it moves away
    • There is something else near the star exerting a gravitational force on it - the exoplanet
    • The time period of the planet's orbit is equal to the period of the Doppler shift
  • Transit method
    • Observing intensity of light output of a star
    • Inclined = don't pass in front of star when observed from earth
    • Transit = when a planet crosses in front of a star
    • Intensity dips slightly
    • If intensity dips regularly it could be a sign that there is an exoplanet orbiting it
    • If there are variations in the regularity of the dips there may be several planets orbiting the same star
    • Have a gravitational effect on the transiting planet
    • The size and orbital period of the planet can be determined from the amount that the intensity falls by and the duration of the dip respectively
  • disadvantage of the transit method
    • limited as it only works if the line of sight to the star is in the plane of the planet’s orbit
    • More likely for planets with small orbits
    • Most orbits are inclined and smaller orbits mean parts of the planet are more likely to cross in front of the star and block some of its light