Please Remember: Turn off Cell Phones and Laptops before class begins – these are distracting to other students. If you insist on talking during the lecture.

Slides:



Advertisements
Similar presentations
Great Ideas in Science: Lecture 9 – Earth as a Planet Professor Robert Hazen UNIV 301 Great Idea: Earth, one of the planets that orbits the Sun, formed.
Advertisements

Solar System Formation – Earth Formation Layers of the Earth Review.
Section 1: Earth’s Interior Who Studies Earth’s Interior?
Planet Earth.
View from the top of the Flatirons (Boulder, CO)
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.
Planetary Science. Why? Since Astronomers find it difficult or impossible to visit most astronomical objects, nearby objects are examined and comparisons/extrapolations.
Please Remember: Last day to withdraw without a grade is Feb. 27th.
This Set of Slides This set of slides covers age and formation of solar system, exoplanets. Units covered: 33, 34.
Origin of the Solar System
The Terrestrial Planets Astronomy 311 Professor Lee Carkner Lecture 9.
Earth Astronomy 311 Professor Lee Carkner Lecture 12.
Announcements Ch. 5 homework will post tonight Test 2 score will post tonight Scores on Mastering Physics continue to be updated Expect to be fully updated.
Earth’s Interior Section 1 Layers of the Earth Section 2
Is There Life Out There? Our Solar System (and beyond) Draw a picture of what you think life would look like on another planet, if it existed. Describe.
Earth’s Interior Section1.
Formation of the Solar System
CH 25.5 Solar System Formation
Solar Nebula Theory Three things we need to examine:
Survey of the Solar System
Solar Nebula Hypothesis
28 Sep 2000ASTR103, GMU, Dr. Correll1 Ch 05--Earth and Moon.
Mrs. McCarthy’s MCAS Review Earth Science 7 th Grade Curriculum –Mapping the Earth –Earth’s Structure –Heat Transfer –Earth’s History –The Earth in the.
Moons Features and Phases Chapter 28. General Information Satellite: a body that orbits a larger body. Seven planets in our solar system have smaller.
The Earth and Its Moon The Earth Solid inner core, liquid outer core atmosphere - 50km thick magnetosphere - charged particles caught in Earth’s magnetic.
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
THE MOON. Definitions Year – time that a planet takes to go around the sun once. Revolution – motion of a body orbiting another body in space Prograde.
Evidence for Early Earth. In order to think about the formation of Earth, there are some assumptions that must be made. Earth today is cooler than early.
Week 10 Day 1 Announcements Grades First iClicker scores have posted (from 4 classes) Participation scores will be up to date after Spring Break .
Earth’s Moon  It takes 27.3 days for the moon to revolve around the Earth relative to a background star (sidereal month).  Because Earth also revolves.
Survey of the Solar System. Introduction The Solar System is occupied by a variety of objects, all maintaining order around the sun The Solar System is.
Earth and Moon Formation and Structure
List all the characteristics you can think of about the moon?
Formation of our solar system: The nebular hypothesis (Kant, 1755) Hydrogen (H), He (He) and “stardust” (heavier elements that were formed in previous.
Plate Tectonics. The Structure of the Earth A thin crust km thick A mantle – has the properties of a solid but it can also flow A core – made.
The Earth and Other Planets
Mechanical waves that travel through the Earth.
The Earth-Moon System The Earth’s Atmosphere
Surface features Earth Terrestrial vs Jovian Formation Other bodies Random $ 200 $ 200$200 $ 200 $ 200 $400 $ 400$400 $ 400$400 $600 $ 600$600 $ 600.
The Moon and Mercury: Airless Worlds Please take your assigned transmitter And swipe your student ID for attendance tracking.
ASTR-1010 Planetary Astronomy Day Announcements Smartworks Chapter 6: Due Today, March 22. Smartworks Chapter 7: Due Friday, March st Quarter.
The Sun & The Solar System. Structure of the Sun The Sun has layers which can be compared to the Earth’s core, mantle, crust, and atmosphere All of these.
Building the Planets. IV. Nebular Capture Nebular capture – growth of icy planetesimals by capturing larger amounts of hydrogen and helium. Led to the.
Chapter 5 Earth and its Moon. The Earth Table 5-1 Some Properties of Earth and the Moon.
1. ALSEP Apollo Lunar Surface Experiments Package Nuclear powered package of instruments left on Moon by Apollo astronauts to measure solar winds, measure.
The Solar System. Solar System the sun and all things orbiting around it, including the eight major planets, their satellites, and all the smaller pieces.
The Structure of the Earth Internal Structure and Heat.
Copyright © 2010 Pearson Education, Inc. Lecture Outline Chapter 5 Earth and Its Moon.
Formation of the Solar System. The Age of the Solar System We can estimate the age of the Solar System by looking at radioactive isotopes. These are unstable.
Chapter 28: The Moon.
12.2 Features of Plate Tectonics  Earth is over 1200 km thick and has four distinct layers.  These layers are the crust, mantle (upper and lower), outer.
Chapter 5: The Earth + the Moon – Part 2. Clicker Question: The Greenhouse effect would not occur if: A: The Earth had no atmosphere. B: The amount of.
Earth Astronomy 311 Professor Lee Carkner Lecture 12.
© Sierra College Astronomy Department Terrestrial Geology Basics.
1 Earth and Other Planets 3 November 2015 Chapter 16 Great Idea: Earth, one of the planets that orbit the Sun, formed 4.5 billion years ago from a great.
Alta High Astronomy Chapter 7 Earth: Our Home in Space.
Origin and Evolution of the Solar System. 1.A cloud of interstellar gas and/or dust (the "solar nebula") is disturbed and collapses under its own.
Notes: Earth/Moon Formation 3/11. 1.Explain the three sources of heat that contributed to the high temperature of the newly formed Earth. (p. 688). The.
The Moon Several theories have been proposed to explain the origin of the Moon.
12.2 Features of Plate Tectonics
The Moon “Jupiter! I did a song! You ain’t got one!” "Camembert?"
Ch. 8: Earth as a Planet.
The study of everything on and in the Earth (including the oceans and the atmosphere), and everything outside of it (the universe). - four major branches.
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
Section 1: Earth’s Moon Preview Key Ideas Exploring the Moon
The Earth.
The Solar System.
Features of Plate Tectonics
Section 1: Earth’s Moon.
3A Objectives Describe the nebular theory in detail.
Presentation transcript:

Please Remember: Turn off Cell Phones and Laptops before class begins – these are distracting to other students. If you insist on talking during the lecture I will insist that you leave. This is getting to be an acute problem with a few students. I will not continue to try to speak over you. Last day to withdraw without a grade is Oct. 3rd

Astronomy Pic of the Day

Solar System Formation, Quick Review Something perturbs an interstellar gas cloud causing it to begin to rotate and contract due to gravitational forces. As the nebula gets smaller is rotates faster (conservation of angular momentum) and therefore must flatten into a disk shape (due to centrifugal force) along its axis of rotation. It also heats up! Star forms at dense center of Nebula. Accretion of dust particles and atoms occurs – forming planetesimals. Planetesimals accreate and form orbits within plane of disk. Planetesimals which are not accreated into the 8 protoplanets are either trapped in the Asteroid Belt or ejected into either the Kuiper Belt (probably by Neptune) or Oort Cloud (probably by Jupiter and/or Saturn). Protoplanets finish accreting nearby material and settle into their current orbits becoming the Planets as we now know them. Finally an intense period of Solar Wind activity follows which expels the remaining gas from the original Nebula from the Solar System.

The Earth From Apollo 17 on Dec. 7, 1972

General Features Mass: M Earth = 6 x kg Radius: R Earth = 6,378 km Density:  = 5,500 kg/m 3 Age: 4.6 billion years Liquid Water! Atmosphere!

Question Why does the Earth have an atmosphere, while the moon does not? A) The Moon is too close to the Earth to have its own atmosphere B) The Moon is not massive enough C) The Moon rotates too quickly on its axis

Escape Speed α √(mass/radius)‏ Earth: 11 km/s Moon: 2.4 km/s Explains why moon has no atmosphere.

Convection (occurs in Troposphere – the part of atmosphere closest to Earth's surface)‏ Convection also occurs when you boil water, or soup. Think of Earth's surface as a boiling pot. Responsible for all weather & contributes to atmospheric heating Heat competes with gravity to keep the atmosphere buoyant! (DEMO)‏

Question The Earth should reradiate all of the energy received from the Sun, giving the Earth a surface temperature of 250 K = -23 o C. Why is the average temperature of Earth so much (about 40 o C) higher? A) Gravity B) Greenhouse effect C) Tilt of Earth on its axis

The Greenhouse Effect Main greenhouse gases are H 2 O and CO 2. If no greenhouse effect, surface would be 40 o C cooler!

Questions What are the major layers in the interior of the Earth? How does density change with depth? What about temperature?

Earth's Internal Structure Mantle is semi-solid rock. Cracks allow material to rise => volcanoes. Core temperature is 6000 K. Outer - Molten. Inner - solid. Metallic How do we obtain information about the structure of the Earth's interior?

Like all waves, seismic waves bend or refract. S-waves are unable to travel in liquid. Measurement of seismic wave gives info on density of Earth's interior and which layers are solid/molten.

Earth's Interior Structure Average density Crust Mantle Core 5,500 kg/m 3 3,000 kg/m 3 5,000 kg/m 3 11,000 kg/m 3 Density increases with depth => "differentiation" (DEMO)‏ Earth must have been molten once, allowing denser material to sink, as it started to cool and solidify. Heating due to (i) bombardment and (ii) radioactivity Bombardment by what? What important result do we see today?

Plates moving at a few cm/year. "Continental drift" or "plate tectonics" Activity on the Earth's Surface

Question What types of geological features or processes would you expect near plate boundaries? What is the driving force behind the motion of the plates?

When plates meet... 1) Head-on collision (Himalayas)‏ 2) "Subduction zone" (one slides under the other)‏ (Andes)‏ 3) "Rift zone" (two plates moving apart)‏ (Mid-Atlantic Ridge)‏ 4) They may just slide past each other (San Andreas Fault)‏ side view top view => mountain ranges, trenches, earthquakes, volcanoes

What causes the drift? Convection! Plates ride on top of convective cells. One cycle takes millions of years => heat loss is extremely slow.

200 million years ago, all the continents were together!

Question What causes the tides?

The Moon = 3,300 kg/m 3 (Earth 5,500 kg/m 3 )‏ = 1/6 that of Earth Mass Radius Density Gravity = M Earth  = 0.27 R Earth

Humans First Visit the Moon - Apollo 11 Mission At 10:56 p.m. eastern daylight time on Sunday, July 20, 1969, Neil Armstrong set his left foot on the moon and spoke the words that were to take their place among the great phrases of history: "That's one small step for a man, one giant leap for mankind." (Movie 1, Movie 2)‏

Tides Tides are due to Moon's gravitational pull being stronger on side of Earth closest to it (Sun also influences tides). Side of Earth closest to Moon feels slightly stronger pull => bulges towards it. Other side feels weaker pull => bulges away compared to rest of Earth. The Earth spins once a day while the bulge always points towards and away from the Moon => two high and two low tides each day.

Tides (cont.)‏

Lunar Structure Moon composed of material very similar to Earth's mantle!

The Lunar Surface ● Dark areas: "maria" More recent lava flows. ● Lighter areas at higher elevation: "highlands". ● Many craters (due to meteorite impacts). Only important source of erosion! ● Highlands have 10x the crater density of maria => Highlands are older! maria highlands

How did the Moon form? We're not quite sure! Two older theories: 1) "Coformation": The Moon and Earth formed out of the same material at the beginning of the Solar System. Problem: Moon has different density and overall composition... 2) "Capture": The Moon was a stray body captured into orbit around Earth. Problem: an extremely unlikely event & parts of compositions are similar...

So now, Impact theory preferred: Early in Solar System, a Mars-sized object hit the forming Earth, ejecting material from the mantle which coalesced to form Moon. Computer simulations suggest this is plausible.