1. Formation of the Universe

2. “In the very beginning, there was a void, a curious form of
vacuum, nothingness containing no space, no time, no
matter, no light, no sound. Yet the laws of nature were in
place and this curious vacuum held potential. A story
logically begins at the beginning, but this story is about the
universe and unfortunately there are no data for the
beginnings—none, zero. We don’t know anything about the
universe until reaches the mature age of a billion of a
trillionth of a second. That is, some very short time after
creation in the big bang. When you read or hear anything
about the birth of the universe, someone is making it up—
we are in the realm of philosophy. Only God knows what
happened at the very beginning.”
--Taken from The God Particle by Leon Lederman, a Nobel Prize winner

3. Cosmology Cosmology is the study of the Nature, Structure, Origin,
And fate of the universe.

4. Universe in a Nutshell

5. Big Bang Theory
The Big Bang Theory was first proposed in the late 1920’s.
It states that there was an infinitely small, infinitely dense point that contained everything that is the universe.
This singularity was incredibly dense and hot.

6. Big Bang Theory
The Big Bang is believed to have occurred between 10 and 15 billion years ago. (Most scientists agree that the universe is 13.7 billion years old.)
Two elements, hydrogen and helium were created in the primordial fireball, along with small amounts of lithium and beryllium.

7. First Three Minutes
First Three Minutes

8. Georges Henri Lemaitre
Late 1920’s
Belgian Astronomer and Jesuit Priest
Known as the “Father of the Big Bang”
First suggested that the universe formed from a singularity but had no evidence.

9. Edwin Hubble 1929 Studied light given off by galaxies.
Noticed that light from most galaxies was shifted to the red end of the electromagnetic spectrum.
Proposed Hubble’s Law after studying these galaxies.

10. Hubble’s Law
The rate at which a galaxy is moving is directly proportional to its distance from us.
In other words, the farther away a galaxy is from us, the faster it travels away from us.
Thus the universe is expanding.

11. Electromagnetic Spectrum

12. Spectral Lines and how they correspond to Absorption lines
Emission Lines
Spectral Lines and how they correspond to Absorption lines

13. Hubble’s Law All Galaxies exhibit redshifts of spectral lines.
More Distant Galaxies Recede Faster

14. The universe is expanding…

15. Cosmic Microwave Background Radiation
Long-wavelength radiation that fills all space.
Can be detected using special antenna. (1% of this can be detected in the static on your TV set.)
George Gamow (1940’s) predicted there should be “echoes” of the Big Bang “explosion.”

16. Bell Laboratories
Penzias and Wilson (1965) were radio astronomers who worked for Bell Telephone Laboratories.
Found a mysterious microwave signal causing background noise in their radio telescope.
The signal came from everywhere.
Arno Penzias Robert Wilson

17. COBE Cosmic Background Explorer (1989)
Probe that looked 15 billion light years into space to detect tiny temperature changes.
These temperature changes were evidence of the heat left over from the Big Bang.

18. WMAP
In June 2001, Wilkinson Microwave Anisotropy Probe (WMAP) captured the “glow” of the Big Bang by detecting temperature changes just like COBE.
WMAP was much more precise.

19. Historical Observations of the CMB and Anisotropy

20. Steady State Theory Opposes the Big Bang Theory
Steady State Theory states that the universe has always been essentially the same as it is today and that it will continue that way forever.

21. Steady State Theory
As matter moves apart, new matter is created to fill the gaps.
Cosmic Background Radiation in the universe ruled out the Steady State Theory.

22. Evidence of the Big Bang
1. The expansion of the universe
Edwin Hubble's 1929 observation that galaxies were generally receding from us provided the first clue that the Big Bang theory might be right.

23. Evidence of the Big Bang
2. The abundance of the light elements H, He, Li
The Big Bang theory predicts that these light elements should have been fused from protons and neutrons in the first few minutes after the Big Bang.
Predicted abundance of elements heavier than hydrogen, as a function of the density of baryons in the universe (expressed in terms of the fraction of critical density in baryons, Omega_B and the Hubble constant)

24. Evidence of the Big Bang
3. The cosmic microwave background (CMB) radiation The early universe should have been very hot. The cosmic microwave background radiation is the remnant heat leftover from the Big Bang.

25. Limitations of the Big Bang
1. Structure in the universe
The Big Bang theory makes no attempt to explain how structures like stars and galaxies came to exist in the universe.

26. Limitations of the Big Bang
2. Fluctuations in the cosmic microwave background (CMB) radiation The temperature of the CMB is observed to vary slightly across the sky. What produced these fluctuations and how do they relate to stars and galaxies?

27. Limitations of the Big Bang
3. The inflationary universe A very short, but especially rapid burst of growth in the very early universe (“inflation”) provides an elegant, yet untested, explanation of the previous puzzles.

28. Big Picture Timeline

30. What’s the Universe Made Of?
4 % Atoms
22% Cold Dark Matter
74% Dark Energy

31. What is Dark Matter?
Dark matter: this generally refers to "exotic" matter that interacts only weakly with ordinary matter. While no such matter has ever been directly observed in the laboratory, its existence has long been suspected.

32. What is Dark Energy?
Dark energy: this is a truly bizarre form of matter, or perhaps a property of the vacuum itself, that is characterized by a large, negative pressure (repelling force). This is the only form of matter that can cause the expansion of the universe to accelerate, or speed up.
Dark Energy Explained

33. WMAP data reveals that its contents include 4
WMAP data reveals that its contents include 4.6% atoms, the building blocks of stars and planets. Dark matter comprises 23% of the universe. This matter, different from atoms, does not emit or absorb light. It has only been detected indirectly by its gravity. 72% of the universe, is composed of "dark energy", that acts as a sort of an anti-gravity. This energy, distinct from dark matter, is responsible for the present-day acceleration of the universal expansion. WMAP data is accurate to two digits, so the total of these numbers is not 100%. This reflects the current limits of WMAP's ability to define Dark Matter and Dark Energy.

34. Fates of the Universe Open Universe Closed Universe Flat Universe
Accelerating Universe

35. Fates of the Universe
Open Universe – little gravity that outward expansion goes on forever
Closed Universe – gravity will eventually halt the expansion and draw everything. Also known as the Big Crunch

36. Fates of the Universe
Flat Universe – expansion slows down but never stops
Accelerating Universe - expansion of the universe will speed up. (Most accepted theory because of dark energy.)

39. Light
A light year is defined as the distance that light travels in one earth year.
Light travels at
300,000 km/s or
186,000 mi/s

40. Remember… Time and Space are Inseparable…
Light travels at a finite speed (3 x 108 m/s)
When you look into the night sky, you look into the past…
The farther out you look, the farther back in time you see…
The sequence of events in the evolution of the universe are “written” in space like an eternal movie…

42. Into the Past Time Required for Light to Travel to the Earth Moon
1.25 seconds
Sun
8.5 minutes
Centrari
4.5 years
Betelgeuse
1200 years
Milky Way
100,000 years
Andromeda
2.2 million years
Virgo Cluster
60 million years
Hydra Super Cluster
3 billion years
Quasars
13 billion years
Cosmic Microwave Background Radiation (CMB)
13.5 billion years