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MICHAEL CHOI SCIENCE HONOURS

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Presentation on theme: "MICHAEL CHOI SCIENCE HONOURS"— Presentation transcript:

1 MICHAEL CHOI SCIENCE HONOURS
THE BIG BANG MICHAEL CHOI SCIENCE HONOURS

2 The darkness of the night
Universe was infinite in age and space = never ending Olber’s Paradox = sky should be bright

3 The darkness of the night
This means the universe has an age = there was a beginning. Infinite Universe Finite Universe In the early 1800’s, it wasn’t clear what was wrong so the word “paradox” was applied.

4 Doppler effect The scrunched up waves  wavelength shorter  higher pitch

5 Doppler effect - light Objects moving towards us  wavelengths shortened, blueshifted, Objects moving away  wavelengths lengthened redshifted.

6 EDWIN HUBBLE Stars and galaxies are moving away from each other
The further they are the faster they are going away INFRARED

7 Quick summary Universe is finite in age but not necessarily in space
Through the Doppler effect = universe is expanding SPACE TIME

8 COSMIC MICROWAVE BACKGROUND RADIATION
13.7 BILLION YEARS AGO COSMIC MICROWAVE BACKGROUND RADIATION WHITE HOT DENSE Electrons Protons subatomic LIGHT CAN’T ESCAPE

9 Cosmic microwave background radiation
PHOTONS. HYDROGEN

10 COSMIC MICROWAVE BACKGOUND RADIATION
FROM ALL DIRECTIONS

11 Cosmic microwave background radiation
IT’S THE AFTERGLOW OF THE BIG BANG

12 Abundance of hydrogen & helium
Easily formed Formed early in the universe Heavier atoms produced in supernovae

13 Dark matter - evidence Undetectable by electromagnetic radiation Light
THERE WASN’T ENOUGH MATTER FOR IT TO BE HELD TOGETHER Undetectable by electromagnetic radiation Light Invisible

14 DARK ENERGY 1998 WE FOUND OUT THAT IT IS ACCELERATING

15 EMPTY SPACE HAS ENERGY. IT PUSHES SPACE ITSELF

16 What will happen to the universe
1. BIG CRUNCH

17 2. Big freeze

18 3. Big rip Galaxies move apart so quickly they break the light-speed barrier

19 1. singularity Expansion not explosion Does the universe have an edge?

20 2. inflation Within 10-43 second
Hundredth of a billionth of a trillionth of a trillionth Size of an atom to size of an orange

21 3. Hot soup Between 10-43 of a second to 3 minutes
It has cooled down from to degrees So that quarks can form into protons and electrons

22 4. 380,000 years after Cool enough to form HYDROGEN AND HELIUM
Light can shine Cosmic microwave background radiation = the afterglow

23 5. First stars 400 milllion years
When they died, they left heavier elements behind

24 6. Galaxies & stars form Gravity makes giant clouds of gas
Which later make galaxies

25 7. Solar system Galaxies cluster together Stars form and die

26 How big is the universe?

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32 The god question? SCIENCE CANT PROVE OR DISPROVE GOD EXISTS
He is outside the universe


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