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Unit 9: Astronomy Earth Science, Chapters 21- 24

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Unit 9: Astronomy. Earth Science, Chapters 21-24. Unit Big Idea/Essential Questions. Entire universe is driven by energy: gravity and electromagnetism. Essential Questions 1.How is the Doppler Effect used to explain movement of the universe? - PowerPoint PPT Presentation

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Page 1: Unit 9: Astronomy

Unit 9: Astronomy

Earth Science, Chapters 21-24

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Unit Big Idea/Essential Questions

Entire universe is driven by energy: gravity and electromagnetism.

Essential Questions1.How is the Doppler Effect used to explain movement of the universe?

2. Explain stellar evolution and how spectroscopes can identify material in a star.

3. How has the view of the universe changed over time?ES Standards: 4.1, 4.2, 4.3

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Key Vocabulary

Aphelion Declination Geocentric Heliocentric Perihelion Retrograde

motion Revolution Rotation

Escape Velocity Maria Solar Nebula Doppler Effect Nuclear Fusion Spectroscopy Absolute/Apparent

magnitude Nebula

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Golden Age of Astronomy Centered in Greece Used geometry and trigonometry Geocentric View and Ptolemaic

System Aristotle- Earth is spherical Eratosthenes- Size of Earth Aristarchus- Distances from Earth Hipparchus- Star Catalogue

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Modern Astronomy

Copernicus and Heliocentric View Tycho Brahe and stellar parallax Kepler and Elliptical orbits Galileo Netwon and Laws of Motion

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Law of Universal Gravitation

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Law of Universal Gravitation Fgravity= G(m1m2/d2) Gravitational Constant (G):

6.67 x 10-11 N*m2/kg2

Calculate force between an object with 50 kg and another object with 50 kg that are .75 m away from each other.

What is the force when the distance is 2500 m?

What happened to the Force of gravity as distance increased?

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Positions in the Sky

2 mapping Systems Constellations Equatorial (declination and right ascension)

Motions of Earth Rotation Revolution

Earth-Moon System

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Origins of the Solar System Theories

Big Bang Nebula

Terrestrial vs. Jovian Planets Earth’s Moon

Theory of formation Lunar Surface

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Signals From Space Electromagnetic Spectrum

Physics of Light Spectrums

Continuous Dark-Line Bright-Line

Doppler Effect Telescopes

Optical Non-Optical

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Sun

Structure Interior Visible Surface: photosphere Atmosphere: chromosphere and corona

Activity Sunspots Prominences Flares

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Stars

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Question of the Day

How do caves form?

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Groundwater

Rate of movement and amount depends on Porosity Permeability Aquitards Aquifers

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Glaciation

Two types Glacial Movement

Zone of accumulation Zone of wastage

Erosion by plucking and abrasion

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Glacial Features via Erosion Glacial Trough Hanging Valleys Cirques Aretes Horns Fjords

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Question of the Day

What are the differences between continental glaciers and alpine glaciers?

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Depositional Features

Till vs. Stratified Drift Glacial Erratics Moranines Outwash Plains Drumlins Eskers Kames Kettle Lakes

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Causes of Glaciation

Plate Tectonics Changes in Earth’s Orbit Changes in output energy from Sun Albedo and Atmosphere composition

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Wind Erosion and Deposition Deflations and Abrasion Loess Sand Dunes

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