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Tuesday November 1, 2011 (The Birth and Evolution of the Earth; Earth’s Spheres)

Tuesday November 1, 2011

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Tuesday November 1, 2011. (The Birth and Evolution of the Earth; Earth’s Spheres). The Launch Pad Tuesday, 11/1/11. List three things that the Earth has but the Moon does not have. an atmosphere. liquid water. life. Announcements. - PowerPoint PPT Presentation

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Page 1: Tuesday November 1, 2011

TuesdayNovember 1, 2011

(The Birth and Evolution of the Earth; Earth’s

Spheres)

Page 2: Tuesday November 1, 2011

The Launch PadTuesday, 11/1/11

List three things that the Earth has but the Moon

does not have.an atmosphere

liquid water

life

Page 3: Tuesday November 1, 2011

Assignment Currently Open

Summative or Formative

Date Issued

Date Due

Date Into

Grade Speed

Last Day

Project – Moon Features Formative 10/18 10/21

Quiz 7 Summative 10/21 10/21 10/25 11/8

Quiz 8 Summative 10/26 10/26 10/27 11/10

Page 4: Tuesday November 1, 2011

AnnouncementsAny remediations that you want to go on this

six-weeks must be done by Friday!

We will have a Quiz tomorrow!

Page 5: Tuesday November 1, 2011

Astrophoto William Souza has caught not just two, but three birds with one stone with this photo he took from Sao Paolo, Brazil. William

captured this photo of the Crescent Moon, Pleiades and Mercury on April 26, 2009.

Page 6: Tuesday November 1, 2011

The Birth of a PlanetThe Nebular Hypothesis assumes a flat, disk shape with the protosun

(pre-Sun) at the center. The inner planets begin to form from

metallic and rocky substances. The larger outer planets began

forming from fragments of ices (H2O, CO2, and other compounds.)

Iron and nickel melted and sank to form the metallic core while rocky

material rose to form the mantle and Earth’s crust.

Page 7: Tuesday November 1, 2011

Early Evolution of Earth Origin of Earth - The Nebular

Hypothesis • Most researchers believe that Earth and

the other planets formed at essentially the same time

• Our solar system evolved from an enormous rotating cloud called the “solar nebula.” (A)• The nebula was composed mostly of

hydrogen and helium.• About 5 billion years ago the nebula

began to contract. (B)• The nebula assumed a flat, disk shape

(accretion disk) with the protosun (pre-Sun) at the center. (C)

• The inner planets begin to form from metallic and rocky clumps. (D)

• The larger outer planets began forming from fragments with a high percentage of ices

• Today (E)

Flattening and spinning. Gravity, shock waves, condensing, “dust bunny” analogy.

Page 8: Tuesday November 1, 2011

The Formation of the Early Earth

Figure 12.5

Page 9: Tuesday November 1, 2011

Early Evolution of EarthFormation of Earth’s Layered Structure

o As Earth formed, the decay of radioactive elements and heat from high-velocity impacts caused the temperature to increase.

o Iron and nickel began to melt and sink toward the center

o Lighter rocky components floated outward, toward the surface

o Gaseous material escaped from Earth’s interior to produce the primitive atmosphere

Page 10: Tuesday November 1, 2011

Cores discovered by tracking seismic

waves traveling through the Earth.

Page 11: Tuesday November 1, 2011

The Earth from the

Moon

Apollo 8Christmas Eve,

1968

The Grand Oasis in Space

Page 12: Tuesday November 1, 2011

Our Home

Fragile

Unique

Vulnerable

Page 13: Tuesday November 1, 2011

Earth’s “Spheres”Geosphere

Hydrosphere CryosphereAtmosphere

BiosphereLithosphere

Asthenosphere Pedosphere

Page 14: Tuesday November 1, 2011

Earth’s “Spheres”Geosphere

the solid matter of the

Earth, as distinct from

the seas, plants,

animals, and surrounding atmosphere

Page 15: Tuesday November 1, 2011

Geosphere

Geosphere

Page 16: Tuesday November 1, 2011

Earth’s “Spheres”Hydrosphere

The ocean is the most prominent feature of the hydrosphere, as it covers

nearly 71% of Earth’s surface and contains about

97% of Earth’s water The hydrosphere also

includes fresh water found in streams, lakes, and

glaciers, as well as that found underground.

Page 17: Tuesday November 1, 2011

Figure 1.10Hydrosphere

Page 18: Tuesday November 1, 2011

Earth’s “Spheres”Cryosphere

This is the frozen part of the Earth's surface, including the polar ice caps,

continental ice sheets, glaciers, sea

ice, and permafrost.

The cryosphere is very important to our

understanding of climate change.

Cryosphere

Page 19: Tuesday November 1, 2011

CryosphereCryosphere

Page 20: Tuesday November 1, 2011

Earth’s “Spheres”Atmosphere

Our atmosphere is the thin, tenuous blanket of air that surrounds Earth.

One-half of the atmosphere lies below 3.5 miles (18 500 feet.)

Our atmosphere shields us from harmful solar rays.

Page 21: Tuesday November 1, 2011

AtmosphereAtmosphere

Page 22: Tuesday November 1, 2011

Earth’s “Spheres”Biosphere

Earth’s biosphere includes all life,

and is concentrated near

the surface in a zone that extends

from the ocean floor upward for

several kilometers into the

atmosphere.

Page 23: Tuesday November 1, 2011

Biosphere

Page 24: Tuesday November 1, 2011

Earth’s “Spheres”Lithosphere The lithosphere is

the rigid outer layer of solid Earth that can be broken.

It includes the crust and the uppermost

mantle, which constitute the hard

and rigid outer layer of the Earth.

Page 25: Tuesday November 1, 2011
Page 26: Tuesday November 1, 2011

Earth’s “Spheres”Asthenosphere

The asthenosphere is

the weaker, hotter, and deeper part of the upper

mantle.

Page 27: Tuesday November 1, 2011

AsthenosphereAsthenosphere

Page 28: Tuesday November 1, 2011

Earth’s “Spheres”Pedosphere

The pedosphere is the uppermost part of the

lithosphere that chemically reacts to the atmosphere,

hydrosphere and biosphere through the soil forming

process.

Page 29: Tuesday November 1, 2011

Pedosphere

Pedosphere