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Title: The Age of Things: Sticks, Stones and the Universe


1
The Age of ThingsSticks, Stones and the Universe
Distances, Redshifts and the Age of the Universe
http//cfcp.uchicago.edu/mmhedman/compton1.html
2
WARNING! Cosmologist talking about Cosmology!
3
Last Time Globular Clusters
11.5 ? 1.3 billion years 12 ? 1 billion
years 11.8 ? 1.2 billion years 14.0 ? 1.2 billion
years 12 ? 1 billion years 12.2 ? 1.8
billion years
Multiple analyses yield ages of 12-13 billion
years, and an uncertainty of about 1 or 2
billion years
M68
M92
M30
M13
NGC362
NGC6752
4
Colors and Spectra
Alberio
1 m
1 km
1 mm
1 ? m
1 nm
1 pm
Visible
600 nm
700 nm
400 nm
500 nm
Wavelength
5
Galaxies
M87
Andromeda
Whirlpool
6
Galaxy Redshifts
(Coutesy of E. Sheldon)
7
The Spectra of different atoms
Sodium
Hydrogen
Calcium
Mercury
Neon
400
500
600
700
Wavelength (nanometers)
8
Galaxy Redshifts
Hydrogen
(Coutesy of E. Sheldon)
9
Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
10
Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
11
Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
12
The Doppler Effect
13
Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
14
Measuring the distance to the stars using Parallax
Background Stars
Nearby Stars
Earth
Earth
Sun
15
Estimating distance with brightness
Sirius
Pollux
Castor
Sirius B
Luminosity Total power emitted by star in
the form of light.
16
Galaxy Distances Cepheids
Large Magellanic Cloud
17
The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Based on Data from Udalski et. al. In Acta
Astronomica Vol 49 (1999) pg 223
18
The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Cepheid in Galaxy Period 10 days Magnitude
24
Cepheid in LMC Period 10 days Magnitude 14
19
The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Cepheid in Galaxy Period 10 days Magnitude
24
Cepheid in LMC Period 10 days Magnitude 14
Same Luminosity
10,000 times fainter
20
The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Cepheid in Galaxy Period 10 days Magnitude
24
Cepheid in LMC Period 10 days Magnitude 14
Same Luminosity
10,000 times fainter
100 times farther away
21
The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Cepheid in Galaxy Period 10 days Magnitude
24
Cepheid in LMC Period 10 days Magnitude 14
Same Luminosity
10,000 times fainter
100 times farther away
150,000 light years away
15 million light years away
22
Galaxy Distances Type Ia Supernova
Luminosity
Supernova 1994D
Days
23
The Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
24
(No Transcript)
25
Now
Then
26
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27
(No Transcript)
28
Hubble Diagram
29
A special point in space implies anisotropies
30
Large scale anisotropies are not observed
Distribution of galaxies from the Sloan Digital
Sky Survey
31
General Relativity
32
Classical Mechanics
An object travels in a straight line at a
constant speed unless acted upon by an outside
force
A force changes the motion of an object by an
amount that depends on its mass
33
Objects move differently due to their composition

-

Unless the force is gravity
34
(No Transcript)
35
Gravity in Classical Mechanics
The more massive object feels a sronger force
The more massive object requires more force to
accelerate it by the same amount
36
Gravity in Classical Mechanics
A
A
B
B
The presence of a massive object exerts a force
that causes all objects to deviate from this path
by the same amount
With no outside forces, all particles take the
path with the shortest distance between two points
37
Gravity in General Relativity
A
A
B
B
The presence of a massive object changes which
path is the shortest distance between the two
points
With no outside forces, all particles take the
path with the shortest distance between two points
38
General Relativity Works
It explains irregularites in Mercurys orbit
It predicted the gravitational lensing of
starlight
39
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40
The Expanding Universe
Now
Then
41
Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
42
Redshifts in an Expanding Universe
Time 1
Time 2
Time 3
43
Scale Factor
a 1
a 0.5
44
Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
45
Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
46
Re-interpreting the Hubble Diagram
Based on Data from Riess et. al. astro-ph/0402512
47
Based on Data from Riess et. al. astro-ph/0402512
48
Re-interpreting the Hubble Diagram
Based on Data from Riess et. al. astro-ph/0402512
49
Extraopolating back to the Big Bang
50
The Big Bang
a 1
a 0.5
a 0
51
Extraopolating back to the Big Bang
52
We need more information to do an accurate
extrapolation
53
No Talk Next Week
June 5 Parametrizing the Age of the Universe
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