1. EARTH’S FORMATION

2. UNIVERSE

3. The Universe Organization: Universe Galaxies Stars Solar Systems
Planets
Moons
Asteroids
Meteoroids

4. The Universe Formation: Big Bang
Initial Mass: Several Billion tons/tablespoon
Age: billion light years
Size: 200 billion galaxies
Contains 50 Billion Trillion Stars
Content:
Dark Energy
Dark Matter
Bright Matter

5. The Big Bang Events Evidence
Begin as a “Singularity” – single condensed form of matter.
Expansion of the singularity – “Inflation”
Matter and antimatter formed
Collision of matter and antimatter creating pure energy
As energy cooled, protons and neutrons began to form, resulting in the formation of Hydrogen.
Other elements formed over time.
A nebulae of gas formed
The nebulae condensed due to gravity to form solid particles which culminated in the formation of stars, planets, etc.
Evidence
Cosmic radiation – Microwaves discovered in 1964
Red Shift – Shift of light spectrum emitted by a star to longer wave lengths which are produced when an object moves away from you – i.e., siren as it passes you.

6. Inventory of Stuff Making up the Universe
Dark Energy %
Dark Matter %
Ordinary Dark Matter %
Ordinary Bright Matter %
Planets %
Reference: Ross, H., 2008.

7. Dark Matter/Energy
5/27/11: A 22-year-old Australian university student has solved a problem which has puzzled astrophysicists for decades, discovering part of the so-called "missing mass" of the universe during her summer break.

8. PLANET FORMATION

9. Formation of the Planets
Nebula Theory – Formation of the planets and stars from a swirling cloud of gas.
Planetesimals (small bodies) joined together through collisions and through the force of gravity to form larger bodies called protoplanets.
Protoplanets’ gravity attracted other planetesimals, collided, and added their masses to the protoplanets.
Eventually, they became very large and condensed to form planets and moons.
The composition of a planet’s atmosphere is based on 2 things:
Size of the planet
Distance of the planet from a neighboring star.

10. NEBULA THEORY Formation of the Planets
The diagram below shows the formation of the Solar System..

11. Our Solar System

12. Formation of Inner Planets
The four protoplanets closest to the sun became Mercury, Venus, Earth, and Mars.
The features of a newly formed planet depended on the distance between the protoplanet and developing sun.
The inner planets are smaller, rockier, and denser than the outer planets. They contain large percentages of heavy elements, such as iron and nickel.
Lighter elements may have been blow or boiled away by radiation from the sun, and because at the temperature of the gases, gravity was not strong enough to hold their gases.

13. Formation of the Outer Planets
The next four protoplanets became Jupiter, Saturn, Uranus, and Neptune.
These outer planets formed far from the sun and therefore were cold. They did not lose their lighter elements, such as helium and hydrogen, or their ices, such as water ice, methane ice, and ammonia ice.
The intense heat and pressure in the planet's interiors melted the ice to form layers of liquids and gases.

14. EARTH FORMATION

15. Earth Formation Earth’s Age: 4.5 Billion Years Old
Four Stages of Formation
Stage One: Hadean – 4.0 to 4.5 BY
formation of Earth’s crust and main bombardment
Stage Two: Archean – 2.5 to 4.0 BY
Formation of Earth’s Land, Water, Atmosphere
Stage Three: Proterozoic – 0.54 to 2.5 BY
Primitive Life, introduction of Photosynthesis – Oxygen Enriched Atmosphere
Stage Four: Phanerazoic – Present to 0.54 BY
Modern Life

16. f08_21_pg221
Hadean
f08_21_pg221.jpg

17. Earth Formation “Hadean Period”
When Earth first formed, it was very hot. During its early history, Earth cooled to form three distinct layers.
In a process called DIFFERENTIATION, denser materials sank to the center, and less dense materials were forced to the outer layers.
The center is a dense core composed mostly of iron and nickel.
Around the core is a very thick layer of iron- and magnesium-rich rock called the mantle.
The outermost layer of Earth is a thin crust of less dense, silica-rich rock.

18. Differentiation of Earth

19. Formation of Earth’s Atmosphere
Earth’s Early Atmosphere
The atmosphere formed because of differentiation.
Earth’s gravity is too weak to hold high concentrations of hydrogen and helium gases and is blown away by solar winds.
Outgassing
Outgassing formed a new atmosphere as volcanic eruptions released large amounts of gases, mainly water vapor, carbon dioxide, nitrogen, methane, sulfur dioxide, and ammonia.
The ozone formed from remaining oxygen molecules after solar radiation caused ammonia and some water vapor to break down.

20. Formation of Earth’s Oceans
The first ocean was probably made of fresh water.
Over millions of years, rainwater fell to Earth and dissolved some of the rocks on land, carrying those dissolved solids into the oceans.
As the water cycled back into the atmosphere through evaporation, some of these chemicals combined to form salts. Through this process, the oceans have become increasingly salty.

21. Outgassing From Volcanic Eruptions

22. Formation of Earth’s Atmosphere
Earth’s Present Atmosphere
The ozone collected in a high atmospheric layer around Earth and shielded Earth’s surface from the harmful ultraviolet radiation of the sun.
Organisms, such as cyanobacteria and early green plants, could survive in Earth’s early atmosphere by using carbon dioxide during photosynthesis.
These organisms produced oxygen as a byproduct of photosynthesis and helped slowly increase the amount of oxygen in the atmosphere.

23. Formation of Earth's Present Atmosphere

24. EARTH FACTS

25. The Ocean’s Effects on the Atmosphere
The ocean affects global temperature by dissolving carbon dioxide from the atmosphere.
Since Earth’s early atmosphere contained less carbon dioxide than today, Earth’s early climate was probably cooler than the global climate is today.

26. Earth Water on Earth Life on Earth
Earth’s unique atmosphere and distance from the sun allow water to exist in a liquid state.
Other planets are too close or far away from the sun,
Life on Earth
Earth is the only known planet that has the proper combination of water, temperature, and oxygen to support life.

27. Atmosphere Thickness: 40 km Troposphere Stratosphere Other layers
Bottom layer
Thickness - 11 km
Weather
Stratosphere
Thickness - 36 km
Ozone Layer
Other layers
Mesophere (Thickness - 34 km)
Thermosphere (Thickness – 14 km)

28. Atmosphere Composition
Nitrogen – %
Oxygen %
Argon %
CO %
Helium %
Methane %
N2O %
CO %
Ozone %

29. THE END