MARS 4 TH ROCK FROM THE SUN MARTIN STEVENS HALESWORTH U3A OCTOBER 2106

Size: px
Start display at page:

Download "MARS 4 TH ROCK FROM THE SUN MARTIN STEVENS HALESWORTH U3A OCTOBER 2106"

Transcription

1 MARS 4 TH ROCK FROM THE SUN MARTIN STEVENS HALESWORTH U3A OCTOBER 2106

2 MARS CAN BE SEEN BY THE NAKED EYE

3 SOME BASICS THINGS WE LIKELY KNOW Fourth plant from the sun -- second smallest after Mercury -- and Pluto was downgraded Named after Roman god of war - Great tune by Holst Often called the Red Planet -- has reddish appearance A terrestrial planet ( rocky) like The Earth Has a thin atmosphere Has impact craters like the moon -- and desserts and polar ice caps as does earth

4 MORE THINGS WE KNOW Goes around the sun quite like earth Has tilt on it s axis like earth causing seasons like earth Has 2 small moons - much smaller than ours Can easily be seen from earth with naked eye - looks red -- only Sun,Moon Jupiter and Venus are brighter

5 MARS AND MOONS RELATIVE SIZES

6 MARS -- PHYSICAL CHARACTERISTICS Approximately half diameter of Earth BUT it s dry land area is very similar to Earth no oceans / rivers / lakes Less dense than Earth about 15% of the Earth volume an 11% of it s mass. -- this results in lower surface gravity about 38% of that on Earth. Red/Orange predominant colour caused by rust (iron oxide) Other colours when you get there -- seen are, golden, brown,tan, greenish- depending on minerals present

7 MARS --- TEMPERATURE Surface Temperature From minus 143C to plus 35C --- mean minus 63Celcius In old money -- minus 226 F to plus 95Fahrenheit -- one of the reasons why there is no liquid water -- more later

8 MARS -- WHAT S IT MADE OF? CORE AND CRUST Structure like Earth - it has a dense metallic core and an outer / overlaid crust Interior core thought to be made primarily of Nickel and Iron -- plus 16% Sulphur Crust -- silica mantel that forms many of the surface features tectonic and volcanic plus collisions But now seems dormant -- no active volcanos / tectonic movement Crust is about 31 miles thick on average Earth crust is about 25miles thick taking size or Earth and Mars into account earth crust is only a third as thick Most abundant elements found in crust -- silicon, oxygen, iron, magnesium, aluminium, calcium, and potassium

9 MARS -- THE SURFACE Largely made up of volcanic rock -- like basalt (Giants Causeway come to mind) Covered in a rusty (iron oxide ) fine grained dust that blows about in the wind more later About 60% of surface shows evidence of external impacts (craters) with likely more evidence hidden below Likely from the so called Late Heavy Bombardment period after formation which all solar system planets were subject to. One theory is that a Pluto sized body impacted some 4 Billion years ago - causing the Borealis Basin which covers 40% of the surface

10 MARS -- GEOLOGICAL HISTORY SHORT VERSION Three primary periods Earliest --Noachian period 4.5 to 3.5 billion years ago surfaces scarred by many impact craters Formation of a volcanic upland Tharsis bulge Flooding by LIQUID water late in the period

11 GEOLOGICAL HISTORY 2 Hesperian period billion years to 2.9/3.3 billion years ago Marked by formation of extensive lava plains -- hence earlier craters underneath! Amazonian period ---- Few impact craters More lava flows CURRENT activity? 2.9/3.3billion years ago to now - not quite dead some evidence of minor lava and water flows, and avalanches from cliffs

12 MARS AND EARTH - TILT AND ROTATION

13 MARS CLIMATE 1 Mars has the most earth like climate in the solar system - due to similar tilts on their rotational axis Martian seasons are about twice those of earth - further from the sun AND takes 2 earth years to go round the Sun. Greater distance from sun than earth ( 1.52) results in just 43% of sunlight falling on it per unit area. More pronounced ellipse in orbit than earth earth more circular - has pronounced effect on climate --- this results in

14 MARS CLIMATE 2 The seasons in the south being more extreme than the seasons in the north The north is therefore milder than it would be if Mars had a more circular orbit Summer temperatures in the south can hit 30C /54F ---- ice would melt! More later Mars has the largest (iron oxide/rust) dust storms in the Solar System vary from small areas to the whole planet Tend to occur when Mars closest to the Sun -- and can increase global temperature

15 POLAR ICE CAPS /2000 North pole South pole

16 MARS -- POLAR CAPS Like Earth Mars has 2 polar ice caps During its winter they are in permanent darkness -- cause 25% of the atmosphere to become slabs of dry (carbon dioxide ) ice. When warming frozen carbon dioxide COs sublimes (to change directly from a solid to a vapour or gas without first melting ) creating enormous winds that sweep off the poles at up to 250 mph Causes Earth like frost and cirrus clouds red dust storms. Both caps compose 70% water ice and then on north cap top a thin layer of seasonal carbon dioxide - dry ice -- south cap has permanent thicker dry ice cover

17 LIFE ON MARS? HABITABILITY -SEARCH FOR LIFE Planetary Habitability ---- the ability of a world to develop environmental conditions favourable to the emergence of life Current understanding is it Favours planets with LIQUID water on their surface 2. Requires the orbit to lie within habitable zone -- for our Solar System extends just beyond Venus to part of the where Mars just dips into on part of its journey around the Sun

18 HABITABILITY 2 BUT Mars thin atmosphere prevents liquid water existing over large area for extended periods. It evaporates as well as mostly too cold Past water flows demonstrate planets habitability potential BUT recent evidence suggests Martian surface water to have then been too salty to support regular terrestrial life Lack of a magnetosphere (Definition of magnetosphere. : a region of space surrounding a celestial object dominated by the object's magnetic field so that charged particles are trapped in it.) and thin atmosphere mean there little heat transfer across the planet -- poor insulation against solar winds and insufficient atmosphere for water to remain as a liquid turns to vapour (steam) Geologically dead (or almost) meaning little chemical mixing /recycling.

19 HABITABILITY 3 -- TIMES PAST? Investigations by two of the Mars Rovers suggest that that Mars was once more habitable than today However whether living organisms ever existed their remains unknown The soil nutrients found would be able to support life BUT it would still need to be shielded from the intense UV light so that only highly reflective or sub surface organics would have been able to have survived

20 MARS THE 2 MOONS

21 MARS THE 2 MOONS Phobos ( Greek - fear /panic) 14 miles across and Deimos (Greek terror/dread) 7.5 miles across which orbit close to the planet Phobos has an unstable descending orbit looks like a recent capture AND may crash onto the Mars surface in 50 million years Asteroid capture remains a long-favoured theory - unlike our Earth Moon which came from Earth Discovered 1877 Composition is more like that of asteroids than Mars

22 MARS EXPLORATION Dozens of spacecraft have been there orbiters, landers and rovers From Russia,USA, Europe and India to study the surface,climate, and geology Currently 7 active probes on or circulating Mars sending data back to Earth Latest from India reached Mars orbit September first successful Asian planetary mission Planned--- Small cubesats now on the way European Space Agency orbiter 2016 and lander 2018 UAE -- planned 2020 /1 orbiter - study the Mars atmosphere Human Missions? -- No active plan has an arrival date before so maybe.

23 MARS - IMPORTANT RECENT OBSERVATIONS 2005 radar data reveals large quantities of water ice and at the poles and elsewhwere 2007 mars rover Spirit finds chemical compounds containing water molecules 2008 Phoenix lander samples water ice in shallow soil 2015 NASA announces presence of briny salt water on surface

24 SOME OLDER OBSERVATIONS - SCIENTIFIC HISTORY Ancient Egyptians recorded a wandering object in sky and by 1534BC aware of its retrograde motion Babylonians astronomers made regular observations - for Mars they worked out it did 42 circuits of the Zodiac every 79 years length of the Martian year 4 th C BC Aristotle worked out Mars went behind our moon - making it further away Known to Chinese astronomers by 4C BC and Indian astronomers by 5C BC 1610 AD - Mars first observed using a telescope --- Galileo

25 MARTIAN CANALS -- LOST IN TRANSLATION 1877 Giovanni - Milan made an early detailed map of Mars - contained what he called cainali - supposedly long straight lines - to which he gave names of well known earth rivers. Canali - mistranslated into canals - a scientific myth was born - the canali later found to be an optical illusion Seasonal changes and apparent canals lead to long held belief in vast seas and vegetation By 1909 better telescopes dismissed this and the canals BUT even up to 1960s papers were written speculating detailed scenarios for the metabolism and chemical cycles for a functioning ecosystem were published. War of the Worlds IS FICTION folks!

26 MARS A THOUGHT TO FINISH ON

27 ANY QUESTIONS?

28 MARS - ANSWERS What is the retrograde motion of Mars caused by? Sometimes the planets appear to change direction in the sky. This retrograde motion is entirely an illusion caused by the Earth passing the slower moving outer planets.

Unit 3 Lesson 4 The Terrestrial Planets. Copyright Houghton Mifflin Harcourt Publishing Company

Unit 3 Lesson 4 The Terrestrial Planets. Copyright Houghton Mifflin Harcourt Publishing Company Florida Benchmarks SC.8.N.1.5 Analyze the methods used to develop a scientific explanation as seen in different fields of science. SC.8.E.5.3 Distinguish the hierarchical relationships between planets

More information

Chapter 17: Mercury, Venus and Mars

Chapter 17: Mercury, Venus and Mars Chapter 17: Mercury, Venus and Mars Mercury Very similar to Earth s moon in several ways: Small; no atmosphere lowlands flooded by ancient lava flows heavily cratered surfaces Most of our knowledge based

More information

UNIT 3: Chapter 8: The Solar System (pages )

UNIT 3: Chapter 8: The Solar System (pages ) CORNELL NOTES Directions: You must create a minimum of 5 questions in this column per page (average). Use these to study your notes and prepare for tests and quizzes. Notes will be turned in to your teacher

More information

What You Already Know

What You Already Know Mars: The Red Planet What You Already Know The Sun is a star, a huge ball of very hot gas that gives off energy. Our Sun is an average star. It is located at the center of the solar system, which consists

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version E of the exam. Please fill in (E). A) This

More information

Mars: The Red Planet. Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos

Mars: The Red Planet. Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos Mars: The Red Planet Roman God of war Blood Reflects 30% of its incident sunlight 2 small moons : Phobos and Deimos Property Earth Mars Radius 6378km 3394km ~ 0.51R E Mass 5.97x10 24 kg 6.42x10 23 kg =

More information

The Main Point. Basic Properties of Mars. Observations. Lecture #19: Mars

The Main Point. Basic Properties of Mars. Observations. Lecture #19: Mars Mars: Overview General properties Telescopic observations Space missions Atmospheric Characteristics Reading: Chapters 7.1 (Mars), 9.4, 10.4 Lecture #19: Mars The Main Point Changes in the Martian surface

More information

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question.

MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. ASTRO 102/104 Prelim 2 Name Section MULTIPLE CHOICE. Choose the one alternative that best completes the statement or answers the question. 1) This is version B of the exam. Please fill in (B). A) This

More information

Learning Objectives. they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field?

Learning Objectives. they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field? The Red Planet Learning Objectives! Contrast the Terrestrial Planets and the Moon. Do they differ in density, composition, atmosphere, surface age, size, geological activity, magnetic field?! Why is Mars

More information

MARS. The Red Planet

MARS. The Red Planet MARS The Red Planet About the Planet Common Name: Mars Mythological Name(s): - Greek: Ares - Roman: Mars Mars is named after the Roman God of War A few Pictures... Distance, Size, and Gravity Compared

More information

Terrestrial Atmospheres

Terrestrial Atmospheres Terrestrial Atmospheres Why Is There Air? An atmosphere is a layer of gas trapped by the gravity of a planet or moon. Here s Earth s atmosphere viewed from orbit: Why Is There Air? If atoms move faster

More information

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time.

Physical Science 1 Chapter 16 INTRODUCTION. Astronomy is the study of the universe, which includes all matter, energy, space and time. INTRODUCTION Astronomy is the study of the universe, which includes all matter, energy, space and time. Although the universe is vast and almost beyond imagination, much is known about its make-up and

More information

Red Planet Mars. Chapter Thirteen

Red Planet Mars. Chapter Thirteen Red Planet Mars Chapter Thirteen ASTR 111 003 Fall 2006 Lecture 11 Nov. 13, 2006 Introduction To Modern Astronomy I Introducing Astronomy (chap. 1-6) Planets and Moons (chap. 7-17) Ch7: Comparative Planetology

More information

Overview of Solar System

Overview of Solar System Overview of Solar System The solar system is a disk Rotation of sun, orbits of planets all in same direction. Most planets rotate in this same sense. (Venus, Uranus, Pluto are exceptions). Angular momentum

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial planets are made mostly of rock and have similar characteristics to Earth. There are four terrestrial

More information

Solar System revised.notebook October 12, 2016 Solar Nebula Theory

Solar System revised.notebook October 12, 2016 Solar Nebula Theory Solar System revised.notebook The Solar System Solar Nebula Theory Solar Nebula was a rotating disk of dust and gas w/ a dense center dense center eventually becomes the sun start to condense b/c of gravity

More information

11/4/2015. Venus and Mars. Chapter 13. Venus and Mars. The Rotation of Venus. The Atmosphere of Venus. The Surface of Venus

11/4/2015. Venus and Mars. Chapter 13. Venus and Mars. The Rotation of Venus. The Atmosphere of Venus. The Surface of Venus Venus and Mars Two most similar planets to Earth: Chapter 13 Venus and Mars Similar in size and mass Same part of the solar system Atmosphere Similar interior structure The Rotation of Venus Almost all

More information

Quiz 3 is available for pickup in front

Quiz 3 is available for pickup in front Quiz 3 is available for pickup in front Extra credit corrections: for up to 4 of the questions you missed: Look up or figure out the correct answer. Write a sentence or two explaining what you did wrong

More information

Inner and Outer Planets

Inner and Outer Planets Inner and Outer Planets SPI 0607.6.2 Explain how the relative distance of objects from the earth affects how they appear. Inner Planets Terrestrial planets are those that are closest to the Sun. Terrestrial

More information

The Solar System. Tour of the Solar System

The Solar System. Tour of the Solar System The Solar System Tour of the Solar System The Sun more later 8 planets Mercury Venus Earth more later Mars Jupiter Saturn Uranus Neptune Various other objects Asteroids Comets Pluto The Terrestrial Planets

More information

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves.

What are terrestrial planets like on the inside? Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds. Seismic Waves. Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds What are terrestrial planets like on the inside? Seismic Waves Vibrations that travel through Earth s interior tell us what Earth is

More information

Physics Homework Set 3 Fall 2015

Physics Homework Set 3 Fall 2015 1) Mercury presents the same side to the Sun 1) A) every third orbit. B) every 12 hours. C) all the time, just like our Moon. D) every other orbit. E) Twice every orbit. 2) Both the Moon and Mercury are

More information

Our Planetary System. Chapter 7

Our Planetary System. Chapter 7 Our Planetary System Chapter 7 Key Concepts for Chapter 7 and 8 Inventory of the Solar System Origin of the Solar System What does the Solar System consist of? The Sun: It has 99.85% of the mass of the

More information

Lecture Outlines. Chapter 10. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc.

Lecture Outlines. Chapter 10. Astronomy Today 8th Edition Chaisson/McMillan Pearson Education, Inc. Lecture Outlines Chapter 10 Astronomy Today 8th Edition Chaisson/McMillan Chapter 10 Mars Units of Chapter 10 10.1 Orbital Properties 10.2 Physical Properties 10.3 Long-Distance Observations of Mars 10.4

More information

Distance of Mercury to the Sun or the Orbital Radius

Distance of Mercury to the Sun or the Orbital Radius Distance of Mercury to the Sun or the Orbital Radius The minimum distance from the Sun to Mercury is about 45866304 kilometers and the maximum distance is about 70006464 kilometers. Space Station One Day

More information

Moons of Sol Lecture 13 3/5/2018

Moons of Sol Lecture 13 3/5/2018 Moons of Sol Lecture 13 3/5/2018 Tidal locking We always see the same face of the Moon. This means: period of orbit = period of spin Top view of Moon orbiting Earth Earth Why? The tidal bulge in the solid

More information

known since prehistoric times almost 10 times larger than Jupiter

known since prehistoric times almost 10 times larger than Jupiter Mercury Venus Earth Mars Jupiter Saturn Uranus Neptune 40.329407-74.667345 Sun Mercury Length of rotation Temperature at surface 8 official planets large number of smaller objects including Pluto, asteroids,

More information

If your plan is for one year, plant rice. If your plan is for 100 years, educate children. Confucius

If your plan is for one year, plant rice. If your plan is for 100 years, educate children. Confucius If your plan is for one year, plant rice. If your plan is for 100 years, educate children. Confucius Test 1 on Wednesday Feb. 20. Sample test and review are On the course web page now. Grades are there

More information

Earth s Atmosphere About 10 km thick

Earth s Atmosphere About 10 km thick 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric properties vary with altitude? Earth s Atmosphere About 10 km thick

More information

The Inner Planets. Chapter 3 Lesson 1. Pages Workbook pages 51-52

The Inner Planets. Chapter 3 Lesson 1. Pages Workbook pages 51-52 The Inner Planets Chapter 3 Lesson 1 Pages 152-159 Workbook pages 51-52 Create the Foldable on pg 159 The solar The planets system The four inner planets Compare and Contrast Question What are planets?

More information

Motion of the planets

Motion of the planets Our Solar system Motion of the planets Our solar system is made up of the sun and the 9 planets that revolve around the sun Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune & Pluto (maybe?)

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds. What is an atmosphere? Earth s Atmosphere. Atmospheric Pressure Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.

Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0. Mercury Named after: Mercury, the fast-footed Roman messenger of the gods. Mean Distance from the Sun: 57,909,175 km (35,983,093.1 miles) or 0.387 astronomical units Diameter: 4,879.4 km (3,031.92 miles)

More information

Jupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons

Jupiter & Saturn. Moons of the Planets. Jupiter s Galilean satellites are easily seen with Earth-based telescopes. The Moons The Moons Jupiter & Saturn Earth 1 Mars 2 Jupiter 63 Saturn 47 Uranus 27 Neptune 13 Pluto 3 Moons of the Planets Galileo (1610) found the first four moons of Jupiter. Total 156 (as of Nov. 8, 2005) Shortened

More information

The Planets. The Terrestrial Planets. Admin. 9/19/17. Key Concepts: Lecture 13. Formulae (will be displayed for you in Midterm 1):

The Planets. The Terrestrial Planets. Admin. 9/19/17. Key Concepts: Lecture 13. Formulae (will be displayed for you in Midterm 1): Admin. 9/19/17 1. Class website http://www.astro.ufl.edu/~jt/teaching/ast1002/ 2. Optional Discussion sections: Tue. ~11.30am (period 5), Bryant 3; Thur. ~12.35pm (end of period 5 and period 6), start

More information

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth

Outline 9: Origin of the Earth: solids, liquids, and gases. The Early Archean Earth Outline 9: Origin of the Earth: solids, liquids, and gases The Early Archean Earth Origin of Earth s Matter The earth is made of recycled elements formed in stars that existed prior to our Sun. Supernova

More information

Terrestrial Bodies of the Solar System. Valerie Rapson

Terrestrial Bodies of the Solar System. Valerie Rapson Terrestrial Bodies of the Solar System Valerie Rapson March 22, 2012 Terrestrial Bodies Many different bodies in the Solar System Gaspra Terrestrial bodies are those with solid surfaces on which one could

More information

What s in Our Solar System?

What s in Our Solar System? The Planets What s in Our Solar System? Our Solar System consists of a central star (the Sun), the main eight planets orbiting the sun, the dwarf planets, moons, asteroids, comets, meteors, interplanetary

More information

Outline 9: Origin of the Earth: solids, liquids, and gases

Outline 9: Origin of the Earth: solids, liquids, and gases Outline 9: Origin of the Earth: solids, liquids, and gases The Early Archean Earth Origin of Earth s Matter The earth is made of recycled elements formed in stars that existed prior to our Sun. Supernova

More information

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Unit 2 Lesson 1 What Objects Are Part of the Solar System? Copyright Houghton Mifflin Harcourt Publishing Company Unit 2 Lesson 1 What Objects Are Part of the Solar System? Florida Benchmarks SC.5.E.5.2 Recognize the major common characteristics of all planets and compare/contrast the properties of inner and outer

More information

Mars ( ) The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled

Mars ( ) The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled The Sun and Planets Lecture Notes 6. Spring Semester 2018 Prof Dr Ravit Helled Mars ( ) Mars is the fourth planet from the Sun and the outermost terrestrial planet. It has a density of 3.93 g/cm3, which

More information

Hubble Telescope Picture of Mars

Hubble Telescope Picture of Mars Information of Mars Mars is the fourth planet from the Sun and is commonly referred to as the Red Planet. The rocks and soil have a red or pink hue due to the iron oxiode (rust) they contain. Hubble Telescope

More information

Planetary Atmospheres (Chapter 10)

Planetary Atmospheres (Chapter 10) Planetary Atmospheres (Chapter 10) Based on Chapter 10 This material will be useful for understanding Chapters 11 and 13 on Jovian planet systems and Extrasolar planets Chapters 4, 5, and 8 on Momentum,

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics Our goals for learning: What is an atmosphere? How does the greenhouse effect warm a planet? Why do atmospheric

More information

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds

The Cosmic Perspective Planetary Atmospheres: Earth and the Other Terrestrial Worlds Chapter 10 Lecture The Cosmic Perspective Seventh Edition Planetary Atmospheres: Earth and the Other Terrestrial Worlds Planetary Atmospheres: Earth and the Other Terrestrial Worlds 10.1 Atmospheric Basics

More information

Chapter 3 The Solar System

Chapter 3 The Solar System Name: Date: Period: Chapter 3 The Solar System Section 1 Observing the Solar System (pp. 72-77) Key Concepts What are the geocentric and heliocentric systems? How did Copernicus, Galileo, and Kepler contribute

More information

Your task for each planet...

Your task for each planet... Solar System Your task for each planet... Slide 1: What type of planet is it? (either rocky terrestrial world, gas giant or ice giant) What is it made of? Does it have any moons? What is its mass relative

More information

The Terrestrial Planets

The Terrestrial Planets The Terrestrial Planets Large Bodies: Earth (1 R E, 1 M E ) Venus (0.95 R E, 0.82 M E ) Small Bodies: Mars (0.53 R E, 0.11 M E ) Mercury (0.38 R E, 0.055 M E ) Moon (0.27 R E, 0.012 M E ) The surfaces

More information

This evening s announcements

This evening s announcements This evening s announcements Homework 3 is graded and available for pickup at entry Quiz 4 will be held this Wednesday, March 12. Coverage: Feb. 25: origin of the solar system (chapter 6) Feb. 27: Earth,

More information

Earth & Space Science ~ The Solar System

Earth & Space Science ~ The Solar System Earth & Space Science ~ The Solar System In e r Sci Uni 11 I. Sun, Earth & Moon A. The Solar System 1. the sun & the objects orbiting it a. incl. 8 planets, other stars, asteroids, meteoroids, dwarf planets,

More information

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds

Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds Chapter 10 Planetary Atmospheres Earth and the Other Terrestrial Worlds What is an atmosphere? 10.1 Atmospheric Basics Our goals for learning:! What is an atmosphere?! How does the greenhouse effect warm

More information

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company

The Outer Planets. Video Script: The Outer Planets. Visual Learning Company 11 Video Script: 1. For thousands of years people have looked up at the night sky pondering the limits of our solar system. 2. Perhaps you too, have looked up at the evening stars and planets, and wondered

More information

Phys 214. Planets and Life

Phys 214. Planets and Life Phys 214. Planets and Life Dr. Cristina Buzea Department of Physics Room 259 E-mail: cristi@physics.queensu.ca (Please use PHYS214 in e-mail subject) Lecture 10. Geology and life. Part 1 (Page 99-123)

More information

CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1)

CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1) Student Sheet 1 CRITICAL THINKING ACTIVITY: INTERPRETING THE GOLDILOCKS EFFECT (1) The Goldilocks Effect is derived from a children's story "The Three Bears" in which a little girl named Goldilocks finds

More information

THE GAS GIANTS JUPITER VENUS MARS EARTH

THE GAS GIANTS JUPITER VENUS MARS EARTH THE GAS GIANTS JUPITER SATURN URANUS NEPTUNE VENUS The temperature at the cloud tops is 200 C while the interior temperatures reach tens of thousands of degrees. The churning of the atmosphere causes temperatures

More information

2010 Pearson Education, Inc.

2010 Pearson Education, Inc. Chapter 10 Planetary Atmospheres: Mars, Venus, Earth What is an atmosphere? An atmosphere is a (usually very thin) layer of gas that surrounds a world. How does the greenhouse effect warm a planet? No

More information

Ch : The Solar System

Ch : The Solar System Ch 16.1-6: The Solar System Hmwk: M: a- I, k- q, s, t, w & x; MC: 1, 5-15; SA: 2, 3, 5-20. Astronomy the scientific study of the universe beyond Earth s atmosphere Universe everything, all energy, matter,

More information

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium

Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium SOLAR SYSTEM NOTES ENERGY TRANSFERS Radiation - a process in which energy travels through vacuum (without a medium) Conduction a process in which energy travels through a medium Convection - The transfer

More information

HNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian

HNRS 227 Fall 2006 Chapter 13. What is Pluto? What is a Planet? There are two broad categories of planets: Terrestrial and Jovian Key Points of Chapter 13 HNRS 227 Fall 2006 Chapter 13 The Solar System presented by Prof. Geller 24 October 2006 Planets Mercury, Venus, Earth, Mars, Jupiter, Saturn, Uranus, Neptune Dwarf Planets Pluto,

More information

After you read this section, you should be able to answer these questions:

After you read this section, you should be able to answer these questions: CHAPTER 16 4 Moons SECTION Our Solar System California Science Standards 8.2.g, 8.4.d, 8.4.e BEFORE YOU READ After you read this section, you should be able to answer these questions: How did Earth s moon

More information

Astronomy. physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1

Astronomy.  physics.wm.edu/~hancock/171/ A. Dayle Hancock. Small 239. Office hours: MTWR 10-11am. Page 1 Astronomy A. Dayle Hancock adhancock@wm.edu Small 239 Office hours: MTWR 10-11am Planetology I Terrestrial and Jovian planets Similarities/differences between planetary satellites Surface and atmosphere

More information

Climate Regulation. - What stabilizes the climate - Greenhouse effect

Climate Regulation. - What stabilizes the climate - Greenhouse effect Climate Regulation - What stabilizes the climate - Greenhouse effect Last time! Processes that shaped Earth: Volcanism, tectonics! How we retain atmospheric molecules ( escape speed )! A magnetic field

More information

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System

Chapter 29. The Solar System. The Solar System. Section 29.1 Models of the Solar System notes Models of the Solar System The Solar System Chapter 29 The Solar System Section 29.1 Models of the Solar System 29.1 notes Models of the Solar System Geocentric: : Earth-centered model of the solar system. (Everything revolves around

More information

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN

SOLAR SYSTEM NOTES. Scientists believe its at least 4.6 billion years old!!! 10/26/2017 ENERGY TRANSFERS RADIATION FROM THE SUN SOLAR SYSTEM NOTES Our Solar System is composed of: 1. The Sun 2. The Planets 3. Asteroids 4. Comets 5. Meteors 6. Natural & Artificial satellites Remember: How old is our Solar System? Scientists believe

More information

Welcome to Class 12: Mars Geology & History. Remember: sit only in the first 10 rows of the room

Welcome to Class 12: Mars Geology & History. Remember: sit only in the first 10 rows of the room Welcome to Class 12: Mars Geology & History Remember: sit only in the first 10 rows of the room What are we going to discuss today? How easily could humans live on Mars? Is there water on Mars? PRS: If

More information

Planet 2. Planet 1 Gas Giant. Planet 3. Earth

Planet 2. Planet 1 Gas Giant. Planet 3. Earth Planet 1 Gas Giant Planet 2 The temperature at the cloud tops is 200 C while the interior temperatures reach tens of thousands of degrees. The churning of the atmosphere causes temperatures of the circulating

More information

Developed in Consultation with Georgia Educators

Developed in Consultation with Georgia Educators Developed in Consultation with Georgia Educators Table of Contents Georgia Performance Standards Correlation Chart........... 7 Performance Standards Chapter 1 Earth and Space.............................

More information

Evolution of the Solar System

Evolution of the Solar System DATE DUE: Name: Ms. Terry J. Boroughs Geology 305 Section: Evolution of the Solar System Instructions: Read each question carefully before selecting the BEST answer or option. Use GEOLOGIC vocabulary where

More information

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars.

Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of the normal stars. Chapter 23 Our Solar System Our Solar System Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths of

More information

Jupiter and its Moons

Jupiter and its Moons Jupiter and its Moons Summary 1. At an average distance of over 5 AU, Jupiter takes nearly 12 years to orbit the Sun 2. Jupiter is by far the largest and most massive planet in the solar system being over

More information

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury.

Name: Date: Hour: 179 degrees celsius. 5% of Earth A 70 pound person would weigh 27 pounds on Mercury. Planet Exploration- http://www.kidsastronomy.com/solar_.htm Mercury 1 87.9 days 58.6 days 57 million Km 465 degrees celsius Minimum -184 degrees celsius 179 degrees celsius Moons Terrestrial or Gaseous?

More information

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week

Today. Events. Terrestrial Planet Atmospheres (continued) Homework DUE. Review next time? Exam next week Today Terrestrial Planet Atmospheres (continued) Events Homework DUE Review next time? Exam next week Planetary Temperature A planet's surface temperature is determined by the balance between energy from

More information

25-Nov-14. The Structure of Earth s Interior. What unique features of Earth are important for life as we know it?

25-Nov-14. The Structure of Earth s Interior. What unique features of Earth are important for life as we know it? What unique features of Earth are important for life as we know it? Surface liquid water Atmospheric oxygen These are obvious Less obvious are: Plate tectonics Climate stability The Structure of Earth

More information

page - Lab 13 - Introduction to the Geology of the Terrestrial Planets

page - Lab 13 - Introduction to the Geology of the Terrestrial Planets page - Lab 13 - Introduction to the Geology of the Terrestrial Planets Introduction There are two main families of planets in our solar system: the inner Terrestrial planets (Earth, Mercury, Venus, and

More information

The Moons of the Solar System

The Moons of the Solar System The Moons of the Solar System By Jordan Smith, Kaitlin McAfee, Erinn Capko, and Ashley Dominguez Survey of the Universe, EMPACTS Project, Spring 2017 Kelly Howe, Instructo4r, Northwest Arkansas Community

More information

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company

Unit 6 Lesson 4 What Are the Planets in Our Solar System? Copyright Houghton Mifflin Harcourt Publishing Company Unit 6 Lesson 4 What Are the Planets in Our Solar System? What other objects are near Earth in this part of space? Earth and millions of other objects make up our solar system. In Our Corner of Space A

More information

Lecture 27: Is There Life on Mars?

Lecture 27: Is There Life on Mars? Lecture 27 Is There Life on Mars? Astronomy 141 Winter 2012 This lecture is about the search for life on Mars The idea of a habitable Mars springs from telescopic observations in the 18 th and 19 th centuries,

More information

Astronomy 1140 Quiz 3 Review

Astronomy 1140 Quiz 3 Review Astronomy 1140 Quiz 3 Review Anil Pradhan October 26, 2016 I The Inner Planets 1. What are the terrestrial planets? What do they have in common? Terrestrial planets: Mercury, Venus, Earth, Mars. Theses

More information

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets

Lecture #11: Plan. Terrestrial Planets (cont d) Jovian Planets Lecture #11: Plan Terrestrial Planets (cont d) Jovian Planets Mercury (review) Density = 5.4 kg / liter.. ~ Earth s Rocky mantle + iron/nickel core Slow spin: 59 days (orbital period = 88 days) No satellites

More information

Read each slide then use the red or some underlined words to complete the organizer.

Read each slide then use the red or some underlined words to complete the organizer. Read each slide then use the red or some underlined words to complete the organizer. 1B Did it start as a bang! 1B The Expanding Universe A. The Big Bang Theory: Idea that all matter began in an infinitely

More information

The Solar System. Presented By; Rahul Chaturvedi

The Solar System. Presented By; Rahul Chaturvedi The Solar System Presented By; Rahul Chaturvedi What s in Our Solar System? Our Solar System consists of a central star (the Sun), the eight planets and their satellites (or moon), thousand of other smaller

More information

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC

OUR SOLAR SYSTEM. James Martin. Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC OUR SOLAR SYSTEM James Martin Facebook.com/groups/AstroLSSC Twitter.com/AstroLSSC It s time for the human race to enter the solar system. -Dan Quayle Structure of the Solar System Our Solar System contains

More information

ASTRO 120 Sample Exam

ASTRO 120 Sample Exam ASTRO 120 Sample Exam 1) If a planet has a reasonably strong magnetic field, we know that a. It is made entirely of iron b. There is liquid nitrogen below the surface c. It can harbor life d. It has a

More information

Mercury and Venus 3/20/07

Mercury and Venus 3/20/07 Announcements Reading Assignment Chapter 13 4 th Homework due today Quiz on Thursday (3/22) Will cover all material since the last exam. This is Chapters 9-12 and the part of 13 covered in the lecture

More information

Explain Distinguish between inner and outer planet characteristics Describe unique features of all the planets

Explain Distinguish between inner and outer planet characteristics Describe unique features of all the planets Loulousis Objectives Explain the nebular hypothesis of the origin of the solar system and describe how the planets formed Distinguish between inner and outer planet characteristics Describe unique features

More information

Unusual Moon Information

Unusual Moon Information Saturn s Numbers Saturn is 1.35 billion km from the Sun minimum. Saturn is 1.5 billion km from the Sun maximum. One day on Saturn takes about 10.67 hours. One full rotation around the sun takes about 29.5

More information

4.2 Detecting Celestial Bodies and the Moon

4.2 Detecting Celestial Bodies and the Moon 4.2 Detecting Celestial Bodies and the Moon Astronomers cannot conduct experiments on celestial objects, they can only observe them at a distance. However, today's technology allows us to see farther into

More information

Inner Planets (Part II)

Inner Planets (Part II) Inner Planets (Part II) Sept. 18, 2002 1) Atmospheres 2) Greenhouse Effect 3) Mercury 4) Venus 5) Mars 6) Moon Announcements Due to technical difficulties, Monday s quiz doesn t count An extra credit problem

More information

37. Planetary Geology p

37. Planetary Geology p 37. Planetary Geology p. 656-679 The Solar System Revisited We will now apply all the information we have learned about the geology of the earth to other planetary bodies to see how similar, or different,

More information

The Jovian Planets (Gas Giants)

The Jovian Planets (Gas Giants) The Jovian Planets (Gas Giants) Discoveries and known to ancient astronomers. discovered in 1781 by Sir William Herschel (England). discovered in 1845 by Johann Galle (Germany). Predicted to exist by John

More information

9. Moon, Mercury, Venus

9. Moon, Mercury, Venus 9. Moon, Mercury, Venus All the heavier elements were manufactured by stars later, either by thermonuclear fusion reactions deep in their interiors or by the violent explosions that mark the end of massive

More information

Module 4: Astronomy The Solar System Topic 3 Content: The Terrestrial Planets Notes Introduction

Module 4: Astronomy The Solar System Topic 3 Content: The Terrestrial Planets Notes Introduction Introduction The four planets closest to the Sun are called "the terrestrial planets." These inner planets are considered to be small and rocky. Although they are all rocky, their varying distances from

More information

Earth as Planet. Earth s s Magnetic Field. The Earth s s Crust. Earth s s Interior

Earth as Planet. Earth s s Magnetic Field. The Earth s s Crust. Earth s s Interior Earth as Planet Earth s s Interior The Earth is a medium size planet with a diameter of 12,756 kilometers (7926 miles) Composed primarily of iron, silicon, and oxygen Nearly circular orbit and just the

More information

Chapter 23. Our Solar System

Chapter 23. Our Solar System Chapter 23 Our Solar System Our Solar System 1 Historical Astronomy Wandering Stars Greeks watched the stars move across the sky and noticed five stars that wandered around and did not follow the paths

More information

Chapter 23 Earth Science 11

Chapter 23 Earth Science 11 Chapter 23 Earth Science 11 Inner planets: Closest planets to the sun A.k.a. terrestrial planets All have a rocky crust, dense mantle layer, and a very dense core Mercury, Venus, Earth, and Mars Outer

More information

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280

Exam# 2 Review. Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280 Exam# 2 Review Exam #2 is Wednesday November 8th at 10:40 AM in room FLG-280 Bring Gator 1 ID card Bring pencil #2 with eraser No use of calculator or any electronic device during the exam We provide the

More information

Opposition and Conjunction

Opposition and Conjunction Opposition and Conjunction Summary 1. Mars is 52% further the Sun having an orbital period of nearly 2 Earth years 2. Mars is much smaller than the Earth being roughly 53% the size, 11% the mass of the

More information

Class Exercise. Today s Class. Overview of Mercury. Terrestrial Planet Interiors. Today s Class: Mercury & Venus

Class Exercise. Today s Class. Overview of Mercury. Terrestrial Planet Interiors. Today s Class: Mercury & Venus Today s Class: Mercury & Venus Homework: Further reading on Venus for next class Sections 10.1 and 10.5 in Cosmic Perspective. Space in the News: 'Frankenstein' Galaxy Surprises Astronomers Presenter:

More information

Terrestrial Planets: The Earth as a Planet

Terrestrial Planets: The Earth as a Planet Terrestrial Planets: The Earth as a Planet In today s class, we want to look at those characteristics of the Earth that are also important in our understanding of the other terrestrial planets. This is

More information