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Announcements

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The distribution of galaxies in space. The discovery that the universe is expanding ... Distances to other galaxies were measured using type I Cepheids ' ... – PowerPoint PPT presentation

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Title: Announcements


1
Announcements
  • Monday, March 26 Midterm II
  • Thursday, March 22, 6-8 pm review session
  • Friday, April 6 Project outline due

2
Lecture 26The expanding universe II How does it
expand?
3
History
  • 1916 Einsteins theory of general relativity
  • 1920-25 spiral nebulae are galaxies like the
    Milky Way
  • 1920-25 Extragalactic distance scale
  • 1929 Hubble redshift-distance relation. Meeting
    with Einstein and Lemaître ? Big Bang model

4
Edwin Hubble (1889-1953)
  • Four major accomplishments
  • in extragalactic astronomy
  • The establishment of the Hubble classification
    scheme of galaxies
  • The convincing proof that galaxies are island
    universes
  • The distribution of galaxies in space
  • The discovery that the universe is expanding

5
Redshift
6
The redshift-distance relation
7
The redshift-distance relation
8
Key results
  • Most galaxies are moving away from us
  • The recession speed v is larger for more distant
    galaxies. The relation between recess velocity v
    and distance d fulfills a linear relation
    v H0 ? d
  • Hubbles measurement of the constant H0
    H0 500 km/s/Mpc
  • todays best fit value of the constant
    H0 65 km/s/Mpc

9
So why was Hubbles original measurement so far
off ?
  • Distance measurement based on the
    period-luminosity relation of Cepheid stars
  • What are Cepheids? They are variable pulsating
    stars

10
So why was Hubbles original measurement so far
off ?
  • There exists a luminosity-period relation for
    Cepheid stars

11
So why was Hubbles original measurement so far
off ?
  • there are two populations of Cepheids (but Hubble
    was not aware of that)
  • type I metal rich stars (disk of galaxies)
  • type II metal poor stars (halo of galaxies)
  • type II Cepheids are less luminous than type I
    Cepheids

12
Consequence
  • Distance scale was calibrated based on type II
    Cepheids
  • Distances to other galaxies were measured using
    type I Cepheids
  • yard stick was systematically to small

13
initial distance 1 length unit final
distance 2 length units recess velocity
1 length unit per time unit
initial distance 2 length units final
distance 4 length units recess velocity
2 length units per time unit
14
Question
  • If all galaxies are moving away from us,
  • does this imply that we are at the center?

Answer
Not necessarily, it also can indicate that the
universe is expanding and that we are at no
special place.
15
Lets go back 15 years ...
16
Lets apply Einsteins equation to the Universe
  • What is the solution of Einsteins equation for a
    homogeneous, isotropic mass distribution?
  • As in Newtonian dynamics, gravity is always
    attractive
  • a homogeneous, isotropic and initially static
    universe is going to collapse under its own
    gravity
  • Alternative expanding universe (Friedmann)

17
A toy universe
  • The model Universe is going to collapse under its
    own gravity

18
Einsteins proposal cosmological constant ?
  • There is a repulsive force in the universe
  • vacuum exerts a pressure
  • empty space is curved rather than flat
  • The repulsive force compensates the attractive
    gravity ? static universe is possible
  • but such a universe turns out to be unstable
    one can set up a static universe, but it simply
    does not remain static
  • Einstein greatest blunder of his life, but is
    it really ?

19
The great synthesis (1930)
  • Meeting by Einstein, Hubble and Lemaître
  • Einstein theory of general relativity
  • Friedmann and Lemaître expanding universe as a
    solution to Einsteins equation
  • Hubble observational evidence that the universe
    is indeed expanding
  • Consequence
  • Universe started from a point? The Big Bang
    Model

20
Announcements
  • Monday, March 26 Midterm II
  • Thursday, March 22, 6-8 pm review session
  • Friday, April 6 Project outline due
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