CHAPTER TWO: THE FORMATION OF THE EARTH – Alison’s …

 

 

Physical Geology Manual, Elementary

CHAPTER TWO:
THE FORMATION OF THE EARTH

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Physical Geology Manual, Elementary

THE FORMATION OF THE UNIVERSE

The ‘Big Bang’ Theory

The ‘Big Bang Theory’ is the most widely accepted theory of the origin of

the universe. About 15 to 20 billion years ago, the primeval atom, a massive collec-

tion of particles and energy, exploded with tremendous force. The particles flew

off into space, gradually coalescing into hydrogen and helium atoms. The gases

expanded and cooled, condensing into galaxies.

This information may be told to children as a story with or without experi-

ments as in ‘The God With No Hands’ by Maria Montessori. The story is in the

History I and Functional Geography manuals.

Presentation: The Formation of the Planets

Gather a group of children and tell the following information in story

form:

The primordial material for the sun and planets is thought to have been a

huge nebular cloud consisting of about 80 percent hydrogen, 15 percent helium,

and a few percent of all other elements. The heavier elements in the frigid cloud of

dust and gases were mostly silicon, aluminum, iron, and calcium. Oxygen, carbon,

and nitrogen were also present in organic compounds.

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About 5 billion years ago, this huge cloud of minute rocky fragments and

gases began to contract under its own gravitational influence. Gradually the atoms

pulled closer and closer together and the cloud became smaller and smaller.

It then developed some component of rotational motion, rotating faster and faster

as it contracted, forming a disk-like shape.The greatest concentration of material

was gravitationally pulled towards the center to form the protosun. The cloud

continued shrinking, causing the center to become hot. The core got hotter and

hotter, until it began to glow with a dim red light. The pressure and temperature

in the core increased, causing a nuclear fusion reaction: hydrogen atoms collided

so violently that they fused together to form helium. The star glowed with a bright

yellow light. It had become our sun.

The rotation of the nebular cloud forming the sun caused it to assume a

flattened disk shape. Within the disk, small contractions occurred, forming the

nuclei of the planets. As the sun got hotter, the temperature in the remainder of

the rotating disk got lower. This allowed metals like iron and nickel with their high

melting temperatures to solidify. Then rock minerals condensed and collided, form-

ing larger and larger bodies until planets, moons, and asteroids formed. The Solar

System began to clear of debris, allowing the sun to shine on the inner planets of

Mercury, Venus, Earth and Mars. Their surface temperatures rose. Because of their

relatively weak gravitational fields, these planets lost hydrogen, helium, ammonia,

methane, and water to the outer planets of Jupiter, Saturn, Uranus, and Neptune.

The colder temperatures of these planets allowed the materials to condense, form-

ing the larger and less dense planets.

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STELLAR NUCLEOSYNTHESIS

Materials:

Piece of black felt 12’ x 3’

8 yellow felt circles with a diameter of 8” representing Hydrogen

7 light pink felt circles with a diameter of 7” representing Helium

6 red felt circles with a diameter of 6” representing Carbon

5 light green felt circles with a diameter of 5” representing Oxygen

4 dark green felt circles with a diameter of 4” representing Neon

3 light blue felt circles with a diameter of 3” representing Magnesium

2 light purple felt circles with a diameter of 2” representing Silicon

1 dark purple felt circle with a diameter of 1” representing Iron

7 yellow felt arrows with a length of 3” and width of 1/2”

3 yellow felt arrows with a length of 6 1/2” and width of 1/2”

8 card stock arrows with a length of 4” and width of 2”: yellow says Hydrogen; light

pink says Helium; red says Carbon; light green says Oxygen; dark green says Neon;

light blue says Magnesium; light purple says Silicon; dark purple says Iron

109 disks with the symbols of the elements written in black

Pictures of stars, nebulae, galaxies

Periodic Table of the Elements

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Presentation:

1.

Say, “Stellar nucleosynthesis is the term for the nuclear reactions taking

place in stars to build the nuclei of the heavier elements. In our sun, the

prime energy producer is the fusion of Hydrogen to Helium, occurring at a

minimum temperature of 5 million degrees F.”

2.

“First, 2 hydrogen nuclei fuse to form deuterium. One proton changes into

one neutron, releasing one neutrino and one positron. This process takes

about 10 billion years.”

3.

Then one deuterium atom fuses with another hydrogen atom to make the

3Helium isotope. Then two 3Helium atoms fuse to form one 4Helium atom

and two 1Hydrogen atoms, releasing energy as heat and light. A Helium

4. Because Hydrogen continues to be produced, there is still a Hydrogen burn-

core forms.

ing shell around the Helium core.

5. Helium burning occurs in older stars with a Helium core and at a temperature

of 100,000,000 K. The star needs to collapse to reach this temperature.

6. Two 4Helium atoms fuse to form one 8Beryllium atom. One 8Beryllium atom

immediately fuses with another 4Helium atom to form one 12Carbon atom,

releasing energy. A Carbon core forms.

7.

4He + 4He –> 8Be

8.

8Be + 4He –> 12C

too quickly.

9. No Carbon was produced in the Big Bang because the temperature dropped

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10. Because Helium continues to be produced, there is still a Helium burning

shell around the Carbon core.

11. Carbon burning occurs in massive stars, four times the mass of our sun and

at a temperature of 600,000,000 K.

12.

12Carbon fuses with 4Helium to form 16Oxygen, releasing energy.

13.

12C + 12C –> 16O + 2 4He

14.

12C + 12C –> 24Mg + alpha particle

15. During the Helium burning process, stars build up an inert core of Car-

bon and Oxygen. When all the Helium is consumed, the core collapses

due to gravitation. Temperature and density increase and Carbon can be

burned.

16. The star becomes a red supergiant.

17. As Carbon burns, Oxygen, Magnesium, and Neon accumulate in a new inert

core. It takes only 1,000 years to burn all the Carbon. Then the core cools

18. Because Carbon continues to be produced, there is still a Carbon burning

and contracts.

shell.

19. Neon burning occurs in very massive stars, eight times the mass of our sun

and at a temperature of 1,200,000,000 K.

20.

20Ne + alpha particle –> 16O + 4He

21.

20Ne + 4He –> 24Mg + alpha particle

22. After all the Carbon in the core is consumed, the core cools down, gravitation

compresses it, and increases the density. Then the temperature increases

so Neon can burn.

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23. Oxygen and Magnesium accumulate in the central core. It takes only a few

years for Neon to be consumed.

24. Because Neon continues to be produced, there is still a Neon burning

shell.

K.

core.

shell.

K.

25. The star is a white dwarf.

26. Oxygen burning occurs in very massive stars at a temperature of 1,500,000,000

27. As Neon is consumed, the core contracts, and becomes denser. The tem-

perature increases so Oxygen can burn.

28. 16O + 16O –> 28Si + 4He

29.

16O + 16O –> 24Mg + 2 4He

30. After six months to one year, all the Oxygen is consumed, leaving a Silicon

31. Because Oxygen continues to be produced, there is still an Oxygen burning

32. Silicon burning occurs in very massive stars at a temperature of 2,700,000,000

33. As Oxygen is consumed, the core contracts and becomes denser. The

temperature increases so Silicon can burn.

34.

28Si + 28Si –> 56Fe + energy

35. After one day, all the Silicon is consumed.

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36.

56Fe (iron) is very stable. No more energy is released, and the star cools

down. The star becomes denser through gravitation. SUPERNOVA! (As

you say this, scatter the discs with all the element symbols on them. Do

not use the element symbols for the elements that are man-made, #43, #61,

#93 – #109.) A huge amount of energy is released and all the other elements

are formed.

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