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The Big Bang Theory (Part II) The Evidence that Supports It Mike Stuckey Warren East High School
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The Big Bang Theory (Part II)

Jan 03, 2016

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The Big Bang Theory (Part II). The Evidence that Supports It. Mike Stuckey Warren East High School. Evidence of the Big Bang. No human was present at the beginning of the universe, so how do we know this is what happened ? What evidence is there ?. Evidence of the Big Bang. - PowerPoint PPT Presentation
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Page 1: The Big Bang Theory (Part II)

The Big Bang Theory (Part II)

The Evidence that Supports It

Mike StuckeyWarren East High School

Page 2: The Big Bang Theory (Part II)

Evidence of the Big Bang

No human was present at the beginning of the

universe, so how do we know this is what happened

?

What evidence is there ?

Page 3: The Big Bang Theory (Part II)

Evidence of the Big Bang

We can’t test our ideas by creating little universes (although this would be

really cool.)

What evidence is there ?

Page 4: The Big Bang Theory (Part II)

Evidence of the Big Bang

To answer this question we must first recall how

science is done.Scientists first create a model

based on observations.

Then scientists make predictions based on these models.

Scientists then try and verify these predictions experimentally or

observationally.

Page 5: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

The most abundant element in the universe should be Hydrogen.

Observation

Although we clearly can’t test the entire universe, all celestial

objects we can see tell us that the most abundant element in each is

hydrogen.

Page 6: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

The concentration of Helium should be greater than 25%.

ObservationDirectly observing evidence of helium is difficult, but when we can measure its

concentration in stars we find that it ranges from 27 to 30 % Helium.

Page 7: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

The universe should be expanding

Edwin Hubble Vesto M. Slipher

Observation

In 1928, Edwin Hubble and Vesto M. Slipher, confirmed separately that the universe is expanding. They

used the Doppler Red Shift of stars and galaxies to prove this.

Page 8: The Big Bang Theory (Part II)

Doppler Effect for Light

When a light source moves away from you, the light it emits shifts toward the red spectrum. This is called Red

Shift.

When a light source moves away from you, the light it emits shifts toward the red spectrum. This is called Red Shift.

When a light source moves away from

you, the light it emits shifts toward the red spectrum. This is called Red

Shift.

When a light source moves away from you, the light it emits shifts

toward the red spectrum. This is called Red

Shift.

When a light source moves away from you, the light it emits

shifts toward the red spectrum. This is called Red Shift.

RED SHIFT

RED SHIFT

Page 9: The Big Bang Theory (Part II)

The galaxies that we observe exhibit the red shift showing that they are moving away from

us.

This observation shows that the universe is expanding!

This evidence supports the Big Bang Theory!

Doppler Effect for Light

Page 10: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

When the universe began, the four fundamental forces were actually one

force.

Page 11: The Big Bang Theory (Part II)

The Fundamental Forces

Gravitational Force

Electromagnetic Force

Nuclear Strong Force

Weak Force

Page 12: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

When the universe began, the four fundamental forces were actually one

force.

Observation

This hasn’t been completely proven, but there is an incredible amount of symmetry between the forces, look at Coulomb’s Law and Newton’s Law of

Gravitation.

In 1983, at Cern Labs, particles were slammed together in their accelerator at extremely high

temperatures and the Electromagnetic Force and the Weak Force were shown to be one force called the Electroweak force.

Page 13: The Big Bang Theory (Part II)

Evidence of the Big BangDirect Observation of the Visible

Universe

It takes a finite amount of time for light to travel a distance. In one second light travel

about 300,000,000 meters.

The distance light travels in a year is called a light-year (ly).

When we look at distant stars or galaxies, we actually are seeing how they looked at some time

in the past.

Page 14: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• It takes light from the Sun approximately 8.3 minutes to reach the Earth

• This means that if we are looking at the Sun we see how it was 8.3 minutes ago. We are looking into the past.

Page 15: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• Alpha Centauri is 4.3 ly away.

• This means it takes light from this star 4.3 years to reach us.

• We are looking 4.3 years into the past.

Page 16: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• Betelgeuse is 1400 ly away.

• This means it takes light from this star 1400 years to reach us.

• We are looking 1400 years into the past.

Page 17: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• The galactic center is 20,000 to 30,000 ly away.

• This means it takes light from the galactic center 20,000 to 30,000 years to reach us.

• We are looking 20,000 to 30,000 years into the past.

Page 18: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• The Andromeda galaxy is 2 million ly away.

• This means it takes light from this galaxy 2 million years to reach us.

• We are looking 2 million years into the past.

Page 19: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• The Hydra Cluster is 3.6 billion ly away.

• This means it takes light from this cluster of galaxies 3.6 billion years to reach us.

• We are looking 3.6 billion years into the past.

Page 20: The Big Bang Theory (Part II)

Direct Observation of the Visible Universe

• This galaxy is 13.2 billion ly away.

• This means it takes light from this galaxy 13.2 billion years to reach us.

• We are looking 13.2 billion years into the past. Not real long after the Big Bang

Page 21: The Big Bang Theory (Part II)

Evidence of the Big Bang

Background Radiation

A crucial moment in the creation of the universe was when the atoms that were

present became neutral and the radiation was able to flow through it and expand

with the universe.

This allowed matter to begin clumping to form the structures we observe in the

universe.

Page 22: The Big Bang Theory (Part II)

Evidence of the Big Bang

Prediction

The temperature of the background radiation should be 2.7 K

Robert Wilson

Arno Penzias

Observation

In 1964, Robert Wilson & Arno Penzias, detected this background

radiation and determined its temperature to be 3.5 K. For this they received the Nobel Prize in Physics. Further experiments have

found that temperature to be 2.7 K.

Page 23: The Big Bang Theory (Part II)

Map of the Background Radiation

In 2003 the WMAP satellite mapped

the cosmic background

radiation, further confirming its

temperature to be 2.7 K.

This map also gave us great

detail about the early universe and it allowed us to refine the

age of the universe to 13.7 billion years.

Page 24: The Big Bang Theory (Part II)

Map of the Background Radiation

This picture shows us how the universe looked 379,000 years

after the Big Bang.