Review 2 Astronomy 150, April 27 th 2005. Moon’s Formation Giant-Impact theory –A Mars-sized object hits the Earth and the Moon is created from the debris.

Slides:



Advertisements
Similar presentations
Chapter 7 Earth and the Terrestrial Worlds
Advertisements

ASTR100 (Spring 2008) Introduction to Astronomy Earth as a Planet Prof. D.C. Richardson Sections
Ch Formation of the Solar System
The Universe. The Milky Way Galaxy, one of billions of other galaxies in the universe, contains about 400 billion stars and countless other objects. Why.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Earth Astronomy 311 Professor Lee Carkner Lecture 12.
Comparing the Planets 10 October Mercury Venus Earth Moon Mars Terrestrial Planets.
Mars Astronomy 311 Professor Lee Carkner Lecture 14.
Goals Explain how Mercury's rotation has been influenced by its orbit around the Sun. Describe how the atmospheres of Venus and Mars differ from one another.
Planetary Geology. Layering of Terrestrial Worlds The process of differentiation separates materials with different densities Dense metals fall.
Astronomy Picture of the Day. Mercury Mass = M Earth Radius = 0.38 R Earth  Surface Temp: K Average distance from Sun =.39 AU Moonlike:
Lunar Facts The moon ended its formation period approximately 4 billion years ago. After the period of formation, the surface of the moon continued to.
ASTR100 (Spring 2008) Introduction to Astronomy Earth as a Planet Prof. D.C. Richardson Sections
Understanding Our Atmosphere
THE INNER PLANETS.
Evolution of the Early Earth
The Solar System.
Chapter 27: Planets of the solar system
Inner Planetary Geology II
Universe Eighth Edition Universe Roger A. Freedman William J. Kaufmann III CHAPTER 10 Our Barren Moon CHAPTER 10 Our Barren Moon.
Lecture Outlines Physical Geology, 14/e Copyright © The McGraw-Hill Companies, Inc. Permission required for reproduction or display. Plummer, Carlson &
Chapter 5 Earth and Moon. What do you think? Will the ozone layer, which is now being depleted, naturally replenish itself? Does the Moon have a dark.
The Moon Formation. Lunar Facts The moon ended its formation period approximately 4 billion years ago. After the period of formation, the surface of the.
Chapter 9 Planetary Geology Earth and the Other Terrestrial Worlds.
Terrestrial Atmospheres Solar System Astronomy Chapter 8.
Homework #5 due next Tuesday, 4:00 pm. Interactions between the surfaces of planets and moon and their interiors play a large role in determining their.
The Earth and Its Moon The Earth Solid inner core, liquid outer core atmosphere - 50km thick magnetosphere - charged particles caught in Earth’s magnetic.
Chapter Part 2 Planets in General Standard Plane Comparative Planetology Hartmann: Chapters 8 Planetary Interiors 9 Planetary Surfaces 10 Planetary.
Terrestrial Planets Earthlike Worlds of Rocks and Metals.
Ch The Earth’s Moon.  Satellite—a body that orbits a larger body.  The moon is earth’s natural satellite.  The moon has weaker gravity (1/6 th.
Review 2 What was the solar nebula? What was it made of? How did gravitational collapse affect the Solar nebula? How does conservation of energy and angular.
Planetary Atmospheres Greenhouse Effect Greenhouse Effect 90 atmospheres!
Exam 2 Postponed Tuesday, November 12 Covers Chapters 7-10, & 14 One sheet of notes with writing on one side only.
(Terrestrial) Planetary Atmospheres II.  Atmospheres consist of exospheres only  Take either of their atmospheres, could “almost store them in a dorm.
Introductory Astronomy Earth is a Planet 1. Inside Earth In molten Earth chemical differentiation. Fe, Ni rich core, Si crust and mantle Density 5500.
Geosphere, Biosphere, Atmosphere and Hydrosphere
Chapter 7 Earth and the Terrestrial Worlds. Mercury craters smooth plains, cliffs.
Lecture 5 6/8/07 AST1001.
1 Inner or Terrestrial Planets All the inner planets formed at the same time. Their composition is also very similar. They lack the huge atmospheres of.
Terrestrial Planets.
Chapter 22 Section 3 Earth’s Moon. Earth vs. Moon 3,475 km 12,756 km Earth has 1 natural satellite  the Moon No specific name other than Moon Unusual.
The Exam results …. Note: Ex1 score = (number correct)/49 You get one ‘bonus’ question due to boo-boo on a question in the 3PMer’s test.
Evolution of Earth’s Spheres
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 6: Due Today, March 22. Smartworks Chapter 7: Due Friday, March st Quarter.
The Moon.
VENUS. “Twin” or “Sister” planet of the earth  similar size, mass, density; interior should also be similar with iron core, mantle, crust But totally.
Earth and the Other Terrestrial Worlds
PLANETARY GEOLOGY. Discuss the factors that affected the geologic processes and formations of the planets Outline the information in the 6 slides Use.
EXPLAIN THE NEBULAR HYPOTHESIS OF THE ORIGIN OF THE SOLAR SYSTEM. DESCRIBE HOW THE PLANETS FORMED DESCRIBE THE FORMATION OF THE LAND, THE ATMOSPHERE, AND.
Mars Images How We Know What We Know Current Spacecraft Mars Odyssey (’01-present) Mars Express (’03-present) Mars Exploration Rovers (’04-present) Mars.
The Terrestrial Planets Chapter 23, Section 2. Mercury: The Innermost Planet  Mercury, the innermost and smallest planet (not counting Pluto), is hardly.
27-1OBJECTIVES Explain the nebular hypothesis of the origin of the solar system Describe how the planets formed Describe the formation of the land, the.
© 2010 Pearson Education, Inc. Chapter 9 Planetary Geology (abridged): Earth and the Other Terrestrial Worlds.
The Terrestrial Planets Mercury, Venus, Earth, Mars.
The Inner Planets.
The Principles of Planetary Geology By: Katie McCormick and Kyle Lennox.
Terrestrial Planets (Chapter 17). Student Learning Objectives Identify & describe each Terrestrial Planet Compare & contrast the Terrestrial planets with.
EARTH’S FORMATION. UNIVERSE The Universe Organization: Organization: Universe Universe Galaxies Galaxies Stars Stars Solar Systems Solar Systems Planets.
Solar System.  Nebular Hypothesis: Solar System was produced by the gravitational collapse of a gas cloud – the remnant of a supernova explosion.  Concentration.
Mars.
Lecture 23.
Evolution of the Early Earth
Chapter 26-27: Test Review Planets, Asteroids, Sun
Venus Second planet from the Sun
Earth’s Interior Structure
The Inner Planets Mercury Venus Earth Mars.
Astronomy 04 The Solar System
Practice Quiz.
Goals Explain how Mercury's rotation has been influenced by its orbit around the Sun. Describe how the atmospheres of Venus and Mars differ from one another.
Earth Astronomy 311 Professor Lee Carkner Lecture 12.
Presentation transcript:

Review 2 Astronomy 150, April 27 th 2005

Moon’s Formation Giant-Impact theory –A Mars-sized object hits the Earth and the Moon is created from the debris –Lack of volatiles – impact was a high energy event and volatile elements evaporated –Lack of iron core – the Moon was created from Earth’s mantle debris – Earth was already differentiated  iron was in the core  low amounts of iron in the ejected debris –Similar Oxygen isotope ratios  similar composition

Mars 4.5OriginOrigin by Accretion 4.5 – 4.0DifferentiationFormation of the original crust 3.9 – 3.8Late Heavy Bombardment Formation of Hellas Basin and the heavily cratered southern highlands 3.8 – 0.6Geological Activity Formation of the Tharsis region and the Northern volcanic plains NowThe Big ChillLow-level cratering and wind erosion Mineral Olivine – quickly dissolves in water  it cannot last for long in wet environments Southern Hemisphere –Mineral Hematite – created in hot, wet environments –Evaporative basins – rocks get saltier as you move down the crater (as the Salt Lake) Lower gravity, lack of plate tectonics  broad, tall shield volcanoes

Venus Thick atmosphere: –no continuous meteoritic bombardment (like on the Moon)  jagged rocks –Lack of simple craters  more complex craters, impact basins Rocks – basalts  geologically active world  lava flows, volcanoes, but no plate tectonics  “blob” tectonics Surface remelts every 0.5 billion years How do we know that it went through 5 planetary stages?

Atmospheres Primary atmospheres – Hydrogen and Helium –Why don’t we have H & He atmospheres? The Sun, combustion/freezing removes atmospheres Secondary atmospheres - main source is outgassing  gasses released when rocks melt Venus – thick, hot atmosphere due to the greenhouse effect  CO 2 stops IR light (heat) emitted from the surface from leaving the planet Earth – very little CO 2  plants! –Rocks also absorb CO 2  rusting –Ozone layer absorbs UV light  UV light does not break up water molecules  we have water and Venus does not Mars – thin atmosphere, no ozone –CO 2 in polar ice caps