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Mr. Kopp’s 8 th Grade Earth Science Welcome
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Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Jan 17, 2016

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Page 1: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Mr. Kopp’s 8th Grade Earth Science

Welcome

Page 2: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Classroom Norms, Rules, and Expectations

• Note takingName: Mr. Kopp Unit: Intro. to Earth Science Topic: What is Earth Science? Date: 9/10/15

Essential Questions:

What is Earth Science?----------------------What are the Branches of Earth Science?

Notes:

-The study of Earth and its place in space-The history of Earth and how it changes over time-------------------------------------------------------------------Earth Science is divided into Meteorology (weather), Astronomy (space), Oceanography (oceans), Geology (solid part of Earth), and Ecology (interaction between life and earth)

Connections to videos, readings, and labs:

Video: “Introduction to Earth Science”

Viewed different things an Earth Scientist might study-Galaxies-Tornadoes-Mountains

Page 3: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

How do we think scientifically?

• 1. Make observations using your 5 senses –

Page 4: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 2. Express any literal findings

• No metaphor or flowery language

• Be specific, accurate

Page 5: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 3. Generate Inferences

• Using prior knowledge and experience to determine a possible explanation

Page 6: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 4. Make real world connections

What are the applications of my inference to other real world events?

Page 7: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 5. Write a conclusion based on factual evidence

Page 8: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

What is the Scientific Method?

Series of steps that help guide scientific study

• Must be repeatable (recipe)• Validates conclusions

Page 9: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

What are the steps of the scientific method?

• 1) Make an Observation in nature• 2) Identify the problem/ask a question• 3) Conduct Research• 4) Form a Hypothesis• 5) Experiment• 6) Collect/Analyze Data• 7) Draw a Conclusion• 8) Present your findings

Page 10: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Fact From Fiction• Scientist classify ideas based upon their ability to

PROVE their ideas using mountains of evidence and repeatable experiments

• Scientific Law – description of what scientists find happening in nature repeatedly and in the same way without exception

• Scientific Theory – a well-tested and widely accepted hypothesis

Page 11: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Scientific Method Keys Terms

• Data – any set of information

• Control – part of an experiment that does not change (used for comparison)

• Variable – part of an experiment that is different

Page 12: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Chapter 1: Introduction to Earth Science

GEOLOGY

ASTRONOMY

OCEANOGRAPHY

METEOROLOGY

ENVIRONMENTAL SCIENCE

Page 13: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

What is Earth Science?

• The name for the group of sciences that study the Earth and its neighbors in space.

Page 14: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
Page 15: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
Page 16: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
Page 17: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
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BIG BANG THEORYFORMATION OF THE UNIVERSE!

Page 19: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
Page 20: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.
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NEBULAR HYPOTHESIS

FORMATION OF THE SOLAR SYSTEM

Page 22: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Formation of the Earth

• NEBULAR HYPOTHESIS– the solar system formed from a giant cloud of gas and dust (nebula)

Page 23: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued• 1) A nearby Giant star explodes in a supernova 5 -7

billion years ago

• 2) The material from this explosion formed a giant cloud of gas and dust – SOLAR NEBULA

Page 24: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued

• 3) The cloud begins to spin due to a gravitational forces

• 4) Materials accrete (come together) at the center as the cloud flattens out

Page 25: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued

• 5) Increased gravity and heat at the center causes immense amounts of material to accrete (come together) at the center (99% of all) – Fusion begins forming our sun

Page 26: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued

• 6) Meanwhile, due to friction, hundreds of larger chunks are forming in the outer portions of the flattened cloud – Planetismals

Page 27: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued • 7) The larger chunks grow faster than the smaller

chunks due to higher gravitational force

• 8) Only the biggest 50 - 100 or so capture all of the other chunks – Protoplanets

Page 28: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 9) The biggest ones have enough gravitational pull to capture the lightest gases such as hydrogen and helium, they are also far enough away from the center (cold enough) to capture icy materials such as ammonia and methane – they become the Outer Planets or Gas Giants

(After the Sun began fusion, solar wind pushed particles outward to the outer planets causing additional growth)

Page 29: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• 10) The smaller, closer ones are not large enough and are too hot to capture many gases. They are called the Inner Planets or Terrestrial Planets

Page 30: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory Continued

• 11) Collisions continue on a massive scale…– A mars-sized object collides with the Earth

forming our moon

12) Many of the moons of the outer planets were captured by the planet’s gravitational pull

Page 31: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Nebular Theory • 1) Supernova creates giant cloud• 2) Giant Cloud (Nebula) begins to spin• 3) Nebula rotates, flattens, accretion in center (protostar)• 4) 100s of planetismals grow in the outer portion of the

disk-like cloud• 5) Fusion begins – Sun is born• 6) 50-100 Proto-planets grow• 7) Massive collisions happen - # of proto-planets decrease• 8) Inner planets remain small and rocky (due to heat)• Outer planet grow huge and gaseous (due to size and cold)• 9) moons are captured or created by explosions

Page 32: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Earth’s Structure

Page 33: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Structure of the Earth• Crust – silicon and oxygen (least

dense)

• Mantle – silicon, oxygen, and magnesium

2,885 km thick, the mantle is 82% of Earth’s volume.

• Outer Core – liquid iron and nickel2,255 km thick Density – 10-12 g/cm3

• Inner Core – solid iron and nickel (most dense)

Radius of 1,220 km. Density – 13 g/cm3

Page 34: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Composition of the crust

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Page 36: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Types of CrustContinental crust – Underlies the continents. –Avg. rock density about 2.7 g/cm3. –Avg. thickness 35-40 km. –Felsic composition (light color)- Avg. rock type = Granite

Oceanic crust – Underlies the ocean basins. –Density about 3.0 g/cm3. –Avg. thickness 7-10 km. –Mafic composition (dark color)- Avg. rock type = Basalt/Gabbro

Page 37: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Origin of the Earth’s Atmosphere and Oceans

• While the Earth was cooling, gasses escaped from the interior (think volcanic eruptions) which became the Atmosphere and eventually rained down to become the oceans

• Source of Heat – radioactive materials, collisions of asteroids/comets

Page 38: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

Shape of the Earth

Oblate Spheroid - • Not a perfect sphere• Flatter at the poles, bulges at

the equator• An object weighs more at the

poles (15N) than it does at the equator (14N)

• The farther an object is from the center of gravity, the less it weighs

Page 39: Mr. Kopp’s 8 th Grade Earth Science Welcome. Classroom Norms, Rules, and Expectations Note taking Name: Mr. KoppUnit: Intro. to Earth ScienceTopic: What.

• Copy down these Earth Facts:• Radius – avg. about 8,000 miles• Circumference• equator is 24,901.55 miles• poles is 24,859.82 miles• Mass – 5,973,000,000,000,000,000,000,000 kg• Density – 5.5 g/cm3• Period of rotation-23 hours 56 min • Equatorial rotation velocity 1,674.4 km/h (465.1 m/s)• Axial tilt 23.5°• Period of Revolution – 365 days 6 hrs 9 min• Average orbital speed 107,200 km/s