Title: The Age of Things: Sticks, Stones and the Universe
1The Age of ThingsSticks, Stones and the Universe
Distances, Redshifts and the Age of the Universe
http//cfcp.uchicago.edu/mmhedman/compton1.html
2WARNING! Cosmologist talking about Cosmology!
3Last 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
4Colors 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
5Galaxies
M87
Andromeda
Whirlpool
6Galaxy Redshifts
(Coutesy of E. Sheldon)
7The Spectra of different atoms
Sodium
Hydrogen
Calcium
Mercury
Neon
400
500
600
700
Wavelength (nanometers)
8Galaxy Redshifts
Hydrogen
(Coutesy of E. Sheldon)
9Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
10Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
11Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
12The Doppler Effect
13Galaxy Redshifts
Hydrogen
Oxygen
(Coutesy of E. Sheldon)
Wavelengths measured in Laboratory
14Measuring the distance to the stars using Parallax
Background Stars
Nearby Stars
Earth
Earth
Sun
15Estimating distance with brightness
Sirius
Pollux
Castor
Sirius B
Luminosity Total power emitted by star in
the form of light.
16Galaxy Distances Cepheids
Large Magellanic Cloud
17The Period-Luminosity Relation of Cepheids
More Luminous
Less Luminous
Based on Data from Udalski et. al. In Acta
Astronomica Vol 49 (1999) pg 223
18The 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
19The 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
20The 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
21The 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
22Galaxy Distances Type Ia Supernova
Luminosity
Supernova 1994D
Days
23The Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
24(No Transcript)
25Now
Then
26(No Transcript)
27(No Transcript)
28Hubble Diagram
29A special point in space implies anisotropies
30Large scale anisotropies are not observed
Distribution of galaxies from the Sloan Digital
Sky Survey
31General Relativity
32Classical 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
33Objects move differently due to their composition
-
Unless the force is gravity
34(No Transcript)
35Gravity 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
36Gravity 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
37Gravity 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
38General Relativity Works
It explains irregularites in Mercurys orbit
It predicted the gravitational lensing of
starlight
39(No Transcript)
40The Expanding Universe
Now
Then
41Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
42Redshifts in an Expanding Universe
Time 1
Time 2
Time 3
43Scale Factor
a 1
a 0.5
44Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
45Re-interpreting the Hubble Diagram
Based on Data from Tonry et. al. astro-ph/0305008
46Re-interpreting the Hubble Diagram
Based on Data from Riess et. al. astro-ph/0402512
47Based on Data from Riess et. al. astro-ph/0402512
48Re-interpreting the Hubble Diagram
Based on Data from Riess et. al. astro-ph/0402512
49Extraopolating back to the Big Bang
50The Big Bang
a 1
a 0.5
a 0
51Extraopolating back to the Big Bang
52We need more information to do an accurate
extrapolation
53No Talk Next Week
June 5 Parametrizing the Age of the Universe