The Expanding Universe - Sonicrknop/php/astronomy/talkslides/modexpuniv.pdf• The three dimensional...
Transcript of The Expanding Universe - Sonicrknop/php/astronomy/talkslides/modexpuniv.pdf• The three dimensional...
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A modern picture of
The Expanding UniverseThe Expanding Universe
Robert KnopAssistant Prof. of Physics & Astronomy
Vanderbilt University
Hypericon II – 2006 June 23
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I. The Shape of the Universe.• Flatland analogy• Non-Euclidean Geometry
II. The Expansion of Space• Measuring Expansion: Redshift• Measuring Expansion Rate
III. A Little Data: how we know• A consistent picture of the Whole Universe (!!)
IV. Reality Check: The “old way” of describing the expansion
V. How did we get here? The Big Bang....
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Flatland
This is the Universe
This dimension doesn't exist(or is something we can't measure, and thus is meaningless)
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Flat (Euclidean) Space:Any triangle, three interior
angles add to 180°
Curved Space: This triangle, three interior angles add to 270°
(In general: >180° : positive curvature<180° : negative curvature)
Flatland (2-dimensional) creatures could measure this curvature without reference to the third dimension we use to describe this here!
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Possible Shapes of the Universe
Closed
Open
Flat
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A model 2-d closed Universe:the surface of a sphere
North/South
East/West
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NowEarlierEven
EarlierEarlier
Still
Just Afterthe
Beginning
Where, on the surface of this sphere, is the center?
Taking the expansion back in timetowards the beginning....
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Distance BetweenGalaxies
Us
SomewhereElse
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Points to notice
• As the Universe expands, galaxies get farther apart, but...
• ...galaxies are not moving through space **
• Galaxies don't expand themselves
• This is probably not the explanation you've heard (i.e. galaxies flying apart with greater speeds at greater differences), but better expresses the modern view of how the Universe works.
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TheVirgo
Cluster
Distance today: 20 Mpc (million parsecs)
Distance in 100 years: 20 Mpc + 1×10-9 Mpc. (Oh well)
Map byJan Wisniewski
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“Lookback” time to Virgo Cluster:
1 parsec = 3.26 lightyears
Light goes 1 lightyear in one year (surprise!)
20 million parsecs means we see the Virgo clutser as it was 65 million years ago.
Can we find something that has expanded along with the Universe over that time????
Yes! Light!
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λ = 4500 Å
λ = 7000 Å
λ = 11,000 Å = 1.1 µm
Blue Light
Red Light
Near-InfraredLight
The Wavelength (λ)of Light.
λ stretches alongwith the Universe
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Cosmological Redshift (z)
z=
Amount wavelength shifts to the red
Original emitted wavelength
Size of Universe at Detection
Size of Universe at Emission=
Size Now
Size Then
Redshift tells us directly how much theUniverse has expanded while the lightwas traveling to us.
1 z=
=observedoriginal
=
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Today
SizeSize Today
1.0
0.5
Back in time Forward in timeTheBig Bang
The Future???
Measuring the Expansion
• Measure distance to get “lookback time” (how long the light took to reach us)
• Measure redshift to get amount of expansion over that time.
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Lookback Times
Object Lookback Time
Sun 8 minutesAlpha Centauri 4 years
Andromeda Galaxy 2 million years
Quasar 3C273at z=0.158
2 billion years
Galaxy at z=1 7 billion years
Age of Universe 13 billion years
Seyfert Galaxy NGC1068 16 million years
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Today
Years in the Past t Years from Today
SizeSize Today
1.0
0.5
LowmassUniverse
HighmassUniverse
Critical MassUniverse
Looking at standard candles (Type Ia supernovae) far enough back in time, we discovered that the expansion of the Universe is accelerating!
AcceleratingUniverse
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A little data...
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A Consistent Picture of the UniverseA Consistent Picture of the Universe
DarkEnergy
DarkMatter
NormalMatter
• 13.7 Billion Years Old
• Flat (Euclidean) Spatial Geometry
• Critical Mass+Energy Density
• Expansion Accelerating
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Today
SizeSize Today
1.0
0.5
The BigCrunch
The Big ChillThe Big RipWhere do we go from here?
It all depends onjust how bizarreDark Energy is!
Years in the Past t Years from Today
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OK, Rob, what about that whole business of farther galaxies moving at higher speeds that we always hear about?
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The Milky Way
A galaxy twiceas far awayincreased itsdistance twiceas much.
Every Point is the Center!
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Δd = change in distance during time of movie (Δt) ∝ d
“Hubble Law”
d t
=H 0d
H0 = current expansion rate of Universe = 71 km/s / Mpc
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Doppler Shift (z)
z=
Amount wavelength shifts to the red
Original emitted wavelength
1+z =Size Now
Size Then
z vc
(For v≪c)
Compare to Cosmological redshift:
For nearby galaxies (out to a few hundred million lightyears), the cosmologic redshift looks just like a doppler shift. The “galaxies flying apart” description is a local Universe approximation.
d dd
= dv td
= 1 vtd
= 1 vd / t
= 1 vc
=
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Summary• The expansion of the Universe is an expansion of space
itself. Galaxies get farther apart, much as do raisins in rising bread, pennies pasted on the surface of an expanding balloon, or paper clips on a stretching elastic band.
• As the Universe expands, the wavelengths of light expand at the same rate.
• The three dimensional space of the Universe can be intrinsically curved, but largescale geometry is flat (Euclidean). (Whew!)
• The expansion of the Universe is accelerating, and indicates that the Universe is filled with Dark Energy.
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Coda: The Big BangIf the Universe is expanding, then in the past it was smaller... far enough back, much smaller.
The Big Bang Theory tells us that the Universe has evolved to its present state from a very condensed and hot state over the course of about 14 billion years.
It does not currently tell us about the actual moment of creation, or what happened before that 14 billion years... there is a point before which our Physics breaks down! (String Theory??)
Evidence for the Big Bang:• Expanding Universe• Cosmic Microwave Background• Fraction of Deuterium and Helium
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A History of the UniverseA History of the Universe
1042 1032 1022
10201025
1012
1015
101
1010
109
105
t (s)
z
Inflation,Grand Unification
... “The beginning?”
T 1013 GeV 108 GeV 1 TeV 100 eV10 MeV
ElectroweakUnification
Protons/NeutronsForm
Elements Form,Cosmic Neutrinos
t
zT
105 104 103 100 10 0
10 kyr 440 kyr 17 Myr 480 Myr 13.7 Gyr30 yr
Matter DominationUniverse Becomes Transparent
Nuclei Capture ElectronsCosmic Microwave Background
First Starsand Quasars You
AreHere
End of GalaxyCluster Formation
2.7 K27 K270 K2700 K
Sun FormsDark Ages
Here beDragons
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Even if the Universe is infinite,the Observable Universe is finite
TheObservableUniverse
“Horizon”
Max. Light
Travel Distance
Youarehere
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The observable Universe, 10-43 secondsafter the Big Bang:
(Actual Size)
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OpaqueUniverse
TransparentUniverse
Cosmic Microwave Background
You Are Here
Farther Away =Further Back in Time
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NowEarlierEven
EarlierEarlier
Still
Just Afterthe
Beginning
Where, on the surface of this sphere, is the center?
Taking this expansion back in timetowards the beginning....
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Extra Slides...
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What do we mean when we say how big something looks?
The angle that it subtends.
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Flat
Closed:Looks Bigger
Open:Looks Smaller
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Spectroscopy
"Fingerprinting" Stars and Galaxies
Light from Star
Spectrometer onTelescope
Light Dispersedby Color
Star or Galaxy Spectrum
Emission and Absorption"Lines"
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Stars: Absorption Lines
Nebulae: Emission lines
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Redshift
Lines in a spectrum
Redshfited Lines