earth science final december 2014 mrs. sagala-riddle

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Earth Science Final December 2014 Mrs. Sagala-Riddle

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Page 1: Earth Science Final December 2014 Mrs. Sagala-Riddle

Earth Science Final

December 2014

Mrs. Sagala-Riddle

Page 2: Earth Science Final December 2014 Mrs. Sagala-Riddle

The Branches of Earth Science

The Branche

s of Earth

Science

Astronomy

Geology

Meteorology

Oceanography

Environmental

Science

Page 3: Earth Science Final December 2014 Mrs. Sagala-Riddle

Earth’s 4 Spheres Atmosphere

Geosphere

Hydrosphere

Biosphere

Page 4: Earth Science Final December 2014 Mrs. Sagala-Riddle

Carbon Cycle

• Photosynthesis• Respiration• Combustion• Erosion• Decomposition

Page 5: Earth Science Final December 2014 Mrs. Sagala-Riddle

Layers of the Earth’s Atmosphere

Page 6: Earth Science Final December 2014 Mrs. Sagala-Riddle

Composition of Earth’s AtmosphereDuring Formation, Outgassing, & Present• During Formation: Hydrogen & Helium

• Outgassing: Outpouring of gases from the earth's interior, Other gases were injected into the atmosphere:• water vapor (produced rain - rivers, lakes, oceans)

• carbon dioxide

• Nitrogen

• Present: 78% Nitrogen 21% Oxygen 1% Other

Page 7: Earth Science Final December 2014 Mrs. Sagala-Riddle

Differences between Inner Planets, Outer Planets, Dwarf Planets, Exoplanets

Inner PlanetsRockyCloser to the sunOrbits the sunFew or no moons/no rings

Outer PlanetsGas planetsFurther from the sunOrbits the sunMany moons & ringsMade of ice & rock

Dwarf PlanetsSmaller than our planets, bigger than asteroidsMedium sized planetsOrbit the sun, not other planetsSphere (round) shaped

ExoplanetsDoes NOT orbit the sun, orbits other starsMost are gas giants

Page 8: Earth Science Final December 2014 Mrs. Sagala-Riddle

Parts of the Sun

Page 9: Earth Science Final December 2014 Mrs. Sagala-Riddle

Life Cycle of Stars like the Sun

• Nebula

• Protostar

• Star like the sun

• Red Giant

• Planetary Nebula

• White Dwarf

Page 10: Earth Science Final December 2014 Mrs. Sagala-Riddle

Life Cycle of a Massive Star

• Nebula

• Protostar

• Massive star

• Red supergiant

• Supernova

• Neutron star

Page 11: Earth Science Final December 2014 Mrs. Sagala-Riddle

Electromagnetic Spectrum

Page 13: Earth Science Final December 2014 Mrs. Sagala-Riddle

Hertzsprung Russell (HR) Diagram

Page 14: Earth Science Final December 2014 Mrs. Sagala-Riddle

Big Bang Theory

• All matter & energy in the universe was compressed into an extremely small

volume that 13 to 15 billion years ago exploded & expanded in all directions.

Page 15: Earth Science Final December 2014 Mrs. Sagala-Riddle

Nebular Hypothesis

• Explains the origin of the solar system.• A rotating nebula cooled & contracted,

throwing off rings of matter that contracted into planets & moons, while the great mass of the condensing nebula became the sun.

Page 16: Earth Science Final December 2014 Mrs. Sagala-Riddle

Giant Impact Hypothesis

• The Moon was formed out of the debris left over from an indirect collision between the Earth and an astronomical body the size of Mars,

• About 4.5 billion years ago

Page 17: Earth Science Final December 2014 Mrs. Sagala-Riddle

Deforestation

• Deforestation is clearing Earth's forests on a massive scale.

• Causes damage to the quality of the land.

• The world’s rain forests could completely vanish in a hundred years at the current rate of deforestation.

Page 18: Earth Science Final December 2014 Mrs. Sagala-Riddle

Greenhouse Effect

Page 19: Earth Science Final December 2014 Mrs. Sagala-Riddle

Red Shift (evidence of the Big Bang Theory)

• Red Shift (Red is the color for longer wavelengths)

• The observed wavelength of the light is longer when objects are moving away from us. The light is shifted towards the red end of the spectrum, RED SHIFT. A force that opposes gravity, pushing galaxies further apart.

Page 20: Earth Science Final December 2014 Mrs. Sagala-Riddle

Blue Shift

Page 21: Earth Science Final December 2014 Mrs. Sagala-Riddle

Parallax

• Shift in position of an object caused by your own motion.

• For example, if you look at some nearby object and move your head a little from side to side, the object looks like it is moving back and forth.

Page 22: Earth Science Final December 2014 Mrs. Sagala-Riddle

Astronomical Unit

• An astronomical unit (au) is a unit of length, roughly the distance from the Earth to the Sun.

Page 23: Earth Science Final December 2014 Mrs. Sagala-Riddle

Light Year

• A light-year is a unit of length used informally to express astronomical distances.

• It is equal to about 6 trillion miles.

• A light-year is the distance that light travels in vacuum in one Julian year.

Page 24: Earth Science Final December 2014 Mrs. Sagala-Riddle

PerihelionAphelion

• Point in the orbit of a planet, asteroid, or comet where it is nearest to the sun.

• Point in the orbit of a planet, asteroid, or comet at which it is furthest from the sun.

Page 25: Earth Science Final December 2014 Mrs. Sagala-Riddle

Constellation

• A constellation is a specific area of the celestial sphere.

• Star Patterns from which the constellations take their names.

• 88 recognized constellations, covering the entire sky.

Page 26: Earth Science Final December 2014 Mrs. Sagala-Riddle

Galaxy

• A massive, gravitationally bound system.

• Consists of stars, stellar remnants, gas, dust & dark matter.