Ques%on: Are there spots on Mars where there are volcanoes and room for a rover to go and land? Importance: It is important to find places to land in
|
|
- Oswin Lyons
- 5 years ago
- Views:
Transcription
1 Ques%on: Are there spots on Mars where there are volcanoes and room for a rover to go and land? Importance: It is important to find places to land in order to find life on Mars.
2 1 st Hypothesis Ø Yes we believe there is room on Mars to land a rover, because there are flat surfaces near the volcanos ends. More references on slides 18 & 19
3 Some of the places that a rover can land. The observa%ons that we have made is that Mars had flat surfaces around the volcanoes. Plus there is a lot of room on the floor of the volcano, so if the volcano is inac%ve the rovers can also land inside the volcano and make its way out.
4 2 nd Hypothesis One reason we think a rover would not be able to land on Mars is because the dust and sand in the air can get into the rover and cause malfunc%ons. For example, you can see the dust molecules in the air.
5 As shown in the picture there is much dirt blowing in the air.
6 Defini%ons v Volcanoes: a vent in the earth's crust through which lava, steam, ashes, etc., are expelled, either con%nuously or at irregular intervals. v A mountain or hill, usually having a cuplike crater at the summit, formed around such a vent from the ash and lava expelled through it.
7 Volcanoes on Mars Some of the volcanic areas for a rover landing on Mars are (Olympus Mons, Alba Mons, Apollinaire Mons, Arsia Mons, Ascraeus Mons, Elysium Mons, and Pavonis Mons) ^^^Olympus Mons ^^^Arsia Mons ^^^Alba Mons
8 Geological Features: Earth V.S. Mars
9 Mars s Geological Features Tectonic features (Ri[ zones) Grada%on (Impact cratering: the size, number, freshness of craters, and rela%on of the other geological features to tell from the Mar%an surfaces) Mass of lava flows Extensional stresses that lead forma%on of great valleys Crisp craters (with upraised rims and steep sides) to make sequence of geological features
10 Earth s Geological Features Volcanism Tectonic plates Impact cratering (Size, numbering, freshness of craters, rela%on of geologic features) Forms of grada%on (observed) Water Energy Origin of Earth system Earth in solar system
11 Astrobiology About study and distribu%on of the origin of the universe Early evolu%on of forming life of our universe Deals with all NASA s space science endeavors, puang together all research in Astrophysics, Earth science, and Heliophysics (planetary science).
12 Con%nue of Astrobiology NASA s Astrobiology Roadmap: Took place in the year of 2008 Provides guidance, research, and technology development of NASA s enterprises of the encompass of space. Contributes diverse scien%sts and technologists from Government, Universi%es, and Private Ins%tu%ons Deals with understanding the nature, and environmental origin of our Universe.
13 Con%nue of Astrobiology NASA s Astrobiology Funding Opportunity Programs: NASA Astrobiology program funds opportuni%es with Science, and Technology of Exploring Planets. NASA also has Astrobiology Funding of solicited independently, and periodically programs.
14 Mars Volcano Data Table
15 Arsia Mons Volcano Eleva%on Graphs Alba Mons Apollinaire Mons Olympus Mons
16 Volcano Eleva%on Graphs Ascraeus Mons Elysium Mons Pavonis Mons
17 Steps on eleva%on graph images: 1. First we opened up JMARS 2. Next, we added new layer Nomenclature. 3. Then we found the type of Mons landmark I needed to search 4. A[er that, we went back to the main menu add new layer Maps by Instrument MOLA MOLA 128ppd Eleva%on Plot numeric data. 5. Next we went back to my JMARS 0E 0N tab, and measured the type of Mons on the screen, then went to the MOLA 128ppd Eleva%on graph. 6. Lastly, it gave us a graph of the eleva%on of that certain volcano.
18 Images of some the volcanoes and the area surrounding it
19 Images of some the volcanoes and the area surrounding it
20 What does MOLA mean? Mars Orbiter Laser Al%meter: they measure by a laser beam, they shoot it into the surface and measure it by how long it takes to come back. This type of measurements uses a color grid to determine the sizes of the eleva%on.
21 Infrared Eleva%on Map Green = Further Research Red = Terminated
22 Introduction Scien%fic Ques%on: What volcanic condi%ons are needed to support extremophiles? Importance?: Scien%st wonder, if Earth and Mars were created the same way and Earth formed life, then wouldn t Mars have formed life too?
23 Introduction pt.2 Interests: This is very interes%ng since evidence of water was found. So this led to our curiosity if life on Mars actually existed. That if volcanoes are on both planets and extremophiles are in Earth s volcanoes, then wouldn t there be some on Mar s volcanoes too?
24 1st Hypothesis Yes, the volcanic condi%ons needed to support extremophiles are very extreme temperatures and ph.
25
26 Background information Biological Features Defini%on: Affec%ng life or living organisms. About Biological Features: Biological features are organism that are microscopic, such as extremophiles.
27 STEPS TO RESEARCH JMARS IMAGES 1. Add new layer 2. Stamps- THEMIS 3. IR- temp range 4. Render and repeat steps 1-4
28 Steps to find Mons 1. New layer 2. Nomenclature 3. Mons 4. Name Mons 5. Record and repeat 1-4
29 About some extremophiles 1.) Extremophiles organisms are primarily Prokaryotic, Archaea, Bacteria, with few Eukaryotic. 2.) They are microorganisms able to live in extreme environments such as hydrothermal vents. 3.) Extremophile produce Extremozymes. 4.) Extremozymes are useful in industrial production.
30 Conclusion Are there spots on Mars where there are volcanoes and room for a rover to go and land? We believe that there are indeed spot/flat surfaces for rovers to land. It is important to find places to land in order to find life on Mars. What volcanic condi%ons are need to support extremophiles? They need extremely high and very low temperature to survive. Extremophiles need high and low ph to survive in the world. Important Scien%st wonder, if Earth and Mars were created the same way and Earth formed life, then wouldn t Mars have formed life too?
31 Ques%ons: What are test that the rover can do? If we find extremophiles, will we find water? What kind of geological features would the rover have to test? How are extremophiles able to survive the extreme condi%ons?
32 Cita%on Oceanservice." Noaa. N.p., Web. 1 Nov <hup://oceanservice.noaa.gov/facts/ extremophile.html>. Hogan, Michael. hup:// N.p., Web. 1 Nov N.p., n.d. Web. 1 Nov <hup://environment.na%onalgeographic.com/environment/natural- disasters/ volcano- profile/>. N.p., Web. 1 Nov <hup:// N.p., n.d. Web. 1 Nov <jmars.asu.edu/>. Burnham, Robert. N.p., n.d. Web. 1 Nov <themis.asu.edu/>. Scallice, Daniella. N.p., Web. 1 Nov <hups://astrobiology.nasa.gov/about- astrobiology/>. Scallice, Daniella. N.p., Web. 1 Nov <hups://astrobiology.nasa.gov/roadmap/>. Scallice, Daniella. N.p., Web. 1 Nov <[hups://astrobiology.nasa.gov/funding/]>.
33 Group Members: Brianna Salas Barron Firdaus Ali Melodi Roane Monique Hedlund Thomas Madrid Simon Lwin Alberto Fernandez
Eleva&on vs. Wind Streaks
Eleva&on vs. Wind Streaks Scien&fic Ques&on Are wind streaks more common in higher or lower eleva&ons on the Southern Hemisphere of Mars? Why This Is Important o Answering this ques&on may help give us
More informationQuestion. Which volcano on the Tharsis region of Mars is the youngest?
Question Which volcano on the Tharsis region of Mars is the youngest? Importance We believe that this question is important and interesting because we don t have any evidence of recent tectonic activity
More information8 th Grade Earth Science Brookhaven Academy
8 th Grade Earth Science Brookhaven Academy Science Question What factors effect lava flows on Mars? Why is this question interesting and important? By studying lava flows on Mars the geology of Mars can
More informationBrookhaven Academy. 8 th Grade Earth Science Final Report
Brookhaven Academy 8 th Grade Earth Science Final Report Introduction and Hypothesis: Science Question: What effect does elevation have on Martian lava flows? Our class was interested in conducting Earth
More informationAre There Plate Tectonics on Mars? 5 th Grade Class of 2013 John Read Middle School Redding, CT 06896
Are There Plate Tectonics on Mars? 5 th Grade Class of 2013 John Read Middle School Redding, CT 06896 Introduction: Are there plate tectonics on Mars? Could plate tectonics explain the formation of Valles
More informationGeologic Features of Mars
Name Purpose Geologic Features of Mars To learn to identify landforms on the surface of Mars and the geological processes that produced them. Introduction In many ways, Mars is similar to Earth. The same
More informationSt. John Bosco Mars Project Essay The question chosen for this project was, what is the relationship between crater
St. John Bosco Mars Project Essay 2012 The question chosen for this project was, what is the relationship between crater diameter and wind streak length. Two hypotheses were formulated to answer this question.
More informationLAVA FLOWS IN THE THARSIS REGION OF MARS: ESTIMATES OF FLOW SPEEDS AND VOLUME FLUXES
LAVA FLOWS IN THE THARSIS REGION OF MARS: ESTIMATES OF FLOW SPEEDS AND VOLUME FLUXES Carolyn Parcheta Department of Geology and Geophysics University of Hawai i at Manoa Honolulu, HI 96822 ABSTRACT The
More informationMars Possible Supervolcanoes
Mars Possible Supervolcanoes By: 5 th Grade GATE Walter Bracken STEAM Academy Supervised by Ms. Sekovski June 2013 Introduction The science question that was researched is, Are volcanic features, such
More informationWhy is this ques0on important and interes0ng? Our ques-on is interes-ng because we want to see if wind veloci-es can vary around Alba Patera.
What is your science ques0on? Can wind streak ra-os be used to determine wind velocity differences in the eleva-on band of 2500-5000m around Alba Patera? Why is this ques0on important and interes0ng? Our
More informationMapping the Surface of Mars Prelab. 1. Explain in your own words what you think a "geologic history" for a planet or moon is?
Prelab 1. Explain in your own words what you think a "geologic history" for a planet or moon is? 2. Describe some of the major features seen on the Martian surface by various spacecraft missions over the
More informationQUESTION IMPORTANCE. It is important to find ice if the idea of humans on Mars would ever become a possibility.
MSIP TEAM KAPPA SCIENCE QUESTION How can crater diameter and rampart diameter ratios of rampart craters be used to find different amounts of ice present in the Northern and Southern parts of Mars? HYPOTHESES
More informationMARS INSIDE AND OUT.
GEOLOGIC SCENE INVESTIGATOR JOURNAL MARS INSIDE AND OUT Explore! Mars Inside and Out Investigator Name www.lpi.usra.edu/education PART I: SCRATCHING THE SURFACE GSI: INSIDE MARS COOLING CUPCAKES AND PLANETS
More informationExamining the Terrestrial Planets (Chapter 20)
GEOLOGY 306 Laboratory Instructor: TERRY J. BOROUGHS NAME: Examining the Terrestrial Planets (Chapter 20) For this assignment you will require: a calculator, colored pencils, a metric ruler, and your geology
More informationIntroduction. Background
Introduction In introducing our research on mars we have asked the question: Is there a correlation between the width of an impact crater and the depth of that crater? This will lead to answering the question:
More informationWhat 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 informationØ How does the length of the volcanic eruption effect the length of the collapsed lava tube?
Ø How does the length of the volcanic eruption effect the length of the collapsed lava tube? Ø Main: The bigger the volcanic eruption the bigger the collapsed lava tube. Ø Alt1: The bigger the volcanic
More information1.2: Observing the Surfaces of Mars and Earth
GEOLOGY ON MARS Unit 1 - Chapter 1-2 Comparing Rocky Planets 1.2: Observing the Surfaces of Mars and Earth Log on to Amplify Geology on Mars Chapter 1.2 In a moment, you will watch a video made by other
More informationWelcome 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 informationInitial Observations and Strategies
STUDENT WORKSHEET 1 Initial Observations and Strategies Name(s) Date Look at the Thermal Emission Imaging System (THEMIS) Daytime Infrared (IR) image mosaic your teacher has given you. You will be investigating
More informationMAPPING THE SURFACE OF MARS
MAPPING THE SURFACE OF MARS What will you learn in this lab? How can we determine the geologic history of a planet or satellite without travelling to the planetary body? In this lab you will create a simple
More informationIntroduction. Background
Introduction Our question was What is the affect of the elevation of an area on the state of the crater found there?. This question is important because it shows us how the weather at each elevation affects
More informationBBC LEARNING ENGLISH 6 Minute English Life on the edge
BBC LEARNING ENGLISH 6 Minute English Life on the edge This is not a word-for-word transcript Hello and welcome to 6 Minute English. I'm And I'm. So, what's your ideal place to be? Curled up on the sofa
More informationGrading Summary: Question 1: 80 points. Question 2: 20 points. Total: 100 points
HOMEWORK #5 Mars & Mercury Due Friday, May 26 th IN CLASS Answers to the questions must be given in complete sentences (except where indicated), using correct grammar and spelling. Please be as brief and
More informationThe Main Points. The View from the Surface. Geology of Mars. Lecture #20: Reading:
Surface of Mars Lecture #20: Geology and Geologic Processes View from the Surface History/Evolution of the surface Reading: Chapter 9.4 The Main Points Mars has had a geologically active past that has
More informationBradley Central High School 4 th Hour Physics. Introduction:
Bradley Central High School 4 th Hour Physics Introduction: Our scientific question is, is there a connection between the location and size of a crater. Our underlying questions are, is there a correlation
More informationFolding. Faulting. Volcanoes
Folding Faulting Volcanoes Most major global mountain ranges were formed by the collision of continental (tectonic) plates Fold mountains are actually formed by crust which have been uplifted and folded
More informationCHANNELS ON MARS. KWL Prior Knowledge/Engagement Activity
CHANNELS ON MARS KWL Prior Knowledge/Engagement Activity In your small group, brainstorm ideas about what you think you know about channels and what questions you have about channels on Mars. You will
More informationLearning 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 informationHighs and Lows Floods and Flows
Highs and Lows Floods and Flows Planetary Mapping Facilitator Guide Becky Nelson Education Specialist The Lunar and Planetary Institute Highs and Lows, Floods and Flows Planetary Mapping Overview In this
More informationType of Exercise: In-Class Activity or Laboratory Exercise.
Using Lava Flows & Volcanic Structures on Mars to Introduce the Concept of Relative Dating in Introductory Courses Audeliz Matias Skidmore College, Saratoga Springs, NY 12866 amatias@skidmore.edu Type
More informationpage - 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 informationIntroduction. width, and location of grabens and tension cracks. The question is important because the answer will show us the
Introduction The question which we based the experience off of was, what was the relationship between the depth, width, and location of grabens and tension cracks. The question is important because the
More informationUNIVERSITY OF MARYLAND ASTRONOMY DEPARTMENT. Mars Cratering. Crater count isochrons of Arsia and Pavonis Mons
UNIVERSITY OF MARYLAND ASTRONOMY DEPARTMENT Mars Cratering Crater count isochrons of Arsia and Pavonis Mons Paul Hearding and Ben McIlwain 5/21/2007 Imagery of Arsia and Pavonis Mons taken by Mars Global
More informationThe 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 informationChapter 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 informationCOSMORPHOLOGY - May 2009
Name COSMORPHOLOGY - May 2009 Geologic landforms Purpose: By studying aerial photographs you will learn to identify different kinds of geologic features based on their different morphologies and learn
More informationMARS. 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 informationOutline 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 informationOutline 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 informationInteriors of Worlds and Heat loss
Interiors of Worlds and Heat loss Differentiation -materials separate into layers by gravity How do we learn about planetary interiors? Measure moment of inertia & average density Observe seismic events
More informationMARS PUBLIC MAPPING PROJECT (MP)2
KWL Prior Knowledge/Engagement Activity In your small group, brainstorm ideas about what you think you know about geologic features that may be found on Mars. Also include what questions you have about
More informationHeight Concordance of Martian Volcanoes Over Time
Height Concordance of Martian Volcanoes Over Time John Moores for PTYS 511 Lunar and Planetary Laboratory, University of Arizona, Tucson AZ Submitted: December 8, 23 Abstract An update to Carr s 1976 paper
More informationWhy. history. features. 1. Fractures. not as wide. the lowered. Graben refers to. complex. This. Mars index_0.html :07
I. Introduction What is your science question? What is the differencee in the depth, width and length of fractures associated with volcanic activity compared to fractures thatt are associated with tectonism
More informationMars for Earthlings. Purpose: Observe and rank potential Earth analogs for Mars planetary study.
LESSON 1: Introduction In Class Activity 1 Mars Analogs Purpose: Observe and rank potential Earth analogs for Mars planetary study. Earth Analogs 1. What do you think scientists mean by an earth analog
More informationVolcano an opening in Earth s crust through which molten rock, gases, and ash erupt and the landform that develops around this opening.
Chapter 9 Volcano an opening in Earth s crust through which molten rock, gases, and ash erupt and the landform that develops around this opening. 3 Conditions Allow Magma to Form: Decrease in pressure
More informationMSIP Proposal Milks Period 4
part of Hebrus Vallis, V11030007, probably lava-formed (http://themis.asu.edu/zoom-20041203a) Tinjar Vallis, V11030007, maybe water-formed? ( http://themis.asu.edu/ zoom-20040519a) MSIP Proposal Milks
More informationESCI 110: Planetary Surfaces Page 3-1. Exercise 3. Surfaces of the Planets and Moons
ESCI 110: Planetary Surfaces Page 3-1 Introduction Exercise 3 Surfaces of the Planets and Moons Our knowledge of the solar system has exploded with the space exploration programs of the last 40 years.
More informationConstructive & Destructive Forces
Constructive & Destructive Forces Intro: Constructive Forces Processes that create landforms. Destructive Forces Processes that destroy landforms. Intro: Constructive Forces Volcanoes Deposition Landslides
More informationName Date. Partners. Comparative Planetology by Mary Lou West after Paul Johnson and Ron Canterna
Name Date Partners Comparative Planetology by Mary Lou West after Paul Johnson and Ron Canterna Purpose : to become familiar with the major features of the planets of the solar system, especially the Earth,
More informationExam# 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 informationMAPPING THE SURFACE OF A PLANET
Written and Developed by: Keith Watt, ASU Mars Education Program Editing by: Paige Valderrama Graff Assistant Director ASU Mars Education Program Sheri Klug Director ASU Mars Education Program SG-SG4 2002
More informationI. Introduction: II. Background:
I. Introduction: Is there a difference between the size of the crater and the ejecta blanket? This question could lead to many different discoveries. When you think about the thousands of craters on mars,
More informationThe 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 informationHighs and Lows, Floods and Flows PLANETARY MAPPING
Highs and Lows, Floods and Flows PLANETARY MAPPING OVERVIEW Teams of students become familiar with the topography of Mars, its geologic features, and patterns of features using a color-coded topographic
More informationHow can solid rock be bent, squished, stretched, and cracked?
AST 105 Intro Astronomy The Solar System MIDTERM II: Tuesday, April 5 4 Processes that Shape Surfaces Volcanism Eruption of molten rock onto surface Impact cratering Impacts by asteroids or comets Tectonics
More informationMoon Formation. Capture Hypothesis Many Hypothesis Fission Hypothesis Double Impact Hypothesis Giant Impact Hypothesis
Moon Formation Capture Hypothesis Many Hypothesis Fission Hypothesis Double Impact Hypothesis Giant Impact Hypothesis Capture Hypothesis Earth seized a pre-formed moon Disproved when lunar samples showed
More informationLESSON 2 THE EARTH-SUN-MOON SYSTEM. Chapter 8 Astronomy
LESSON 2 THE EARTH-SUN-MOON SYSTEM Chapter 8 Astronomy OBJECTIVES Investigate how the interaction of Earth, the Moon, and the Sun causes lunar phases. Describe conditions that produce lunar and solar eclipses.
More informationMars for Earthlings. Purpose: Recognize the purpose and need for understanding the scale and context of various remote sensing imaging techniques.
LESSON 4: Remote Sensing Mars In-Class Activity 1 Scale and Context Purpose: Recognize the purpose and need for understanding the scale and context of various remote sensing imaging techniques. Study the
More informationRed 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 informationASTRONOMY 340 FALL September 2007 Class #6-#7
ASTRONOMY 340 FALL 2007 25 September 2007 Class #6-#7 Review Physical basis of spectroscopy Einstein A,B coefficients probabilities of transistions Absorption/emission coefficients are functions of ρ,
More information11/4/2015. 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 informationClass 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 informationASTR 380 Possibilities for Life in the Inner Solar System
ASTR 380 Possibilities for Life in the Inner Solar System ASTR 380 Midterm Test Results Generally people did well: 100-90 = A = 19 people 89 80 = B = 19 people 79 70 = C = 9 people 69 60 = D = 0 < 60 =
More informationGrades 9-12: Earth Sciences
Grades 9-12: Earth Sciences Earth Sciences...1 Earth s Place in the Universe...1 Dynamic Earth Processes...2 Energy in the Earth System...2 Biogeochemical cycles...4 Structure and Composition of the Atmosphere...4
More informationVolcanoes. Presented by Kesler Science
Presented by Kesler Science Essential Questions: 1. What are the parts of a volcano? 2. What are the four types? 3. What processes form volcanoes? 4. Where are volcanoes located on earth? What is a Volcano?
More informationMARS STUDENT IMAGING PROJECT FINAL REPORT ASU MARS EDUCATION PROGRAM Waubonsie Valley High School Period School Year
I. Introduction What is your science question? What effect do the polar ice caps have on craters in the rock strata? Why is this question important and interesting? This question is important for the following
More informationLecture 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 informationForces that Shape the Land. Plate Tectonics
Forces that Shape the Land Plate Tectonics Directions: This packet goes along with my plate tectonics powerpoint. After viewing the powerpoint, students are to complete this activity sheet. 1. Start by
More informationWhat is Crater Number Density?
Ronald Wilhelm & Jennifer Wilhelm, University of Kentucky 2008 What is Crater Number Density? REAL Curriculum Crater Number Density Today we will learn some math that is necessary in order to learn important
More informationToday. Events. Terrestrial Planet Geology. Fall break next week - no class Tuesday
Today Terrestrial Planet Geology Events Fall break next week - no class Tuesday When did the planets form? We cannot find the age of a planet, but we can find the ages of the rocks that make it up. We
More information2. Terrestrial Planet G 9. Coulomb Force C 16. Babcock model Q. 3. Continuous Spectrum K 10. Large-impact hypothesis I 17.
Astronomy 1 S 16 Exam 1 Name Identify terms Label each term with the appropriate letter of a definition listed 1. Spectral line R 8. Albedo H 15. helioseismology E 2. Terrestrial Planet G 9. Coulomb Force
More informationTectonic Forces Simulation: Volcanoes Activity One
Tectonic Forces Simulation: Volcanoes Activity One Introduction Volcanoes form above vents or cracks in the earth's crust. When a volcano erupts, magma is forced up through the cracks - sending lava, ash,
More informationTopographic variability on Mars: Implications for lava flow modeling
JOURNAL OF GEOPHYSICAL RESEARCH, VOL. 112,, doi:10.1029/2006je002879, 2007 Topographic variability on Mars: Implications for lava flow modeling L. S. Glaze 1 and S. M. Baloga 1 Received 7 December 2006;
More informationChapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds
Chapter 9 Planetary Geology: Earth and the Other Terrestrial Worlds 9.1 Connecting Planetary Interiors and Surfaces Our goals for learning What are terrestrial planets like on the inside? What causes geological
More informationEarth & Space Science Exploration of Extreme Environments: Volcanoes
a place of mind F A C U L T Y O F E D U C A T I O N Department of Curriculum and Pedagogy Earth & Space Science Exploration of Extreme Environments: Volcanoes Science and Mathematics Education Research
More informationEarth, the Lively* Planet. * not counting the life on the planet!
Earth, the Lively* Planet * not counting the life on the planet! What We Will Learn Today What are planet Earth s features? What processes shape planetary surfaces? How does Earth s surface move? How did
More informationStrand 1: Inquiry Process
Strand 1: Inquiry Process Concept 1: Observations, Questions, and Hypotheses Formulate predictions, questions, or hypotheses based on observations. Locate appropriate resources. PO 1. Formulate questions
More informationPSRD: Recent Activity on Mars: Fire and Ice
of 8 posted January 31, 2005 Recent Activity on Mars: Fire and Ice --- New images from Mars Express show evidence of recent volcanic and glacial activity on Mars, consistent with what we know from Martian
More informationAstrobiology: The Semester in Review
A Universe of Life Astrobiology: The Semester in Review Honors 228 with Dr. Harold Geller Searching for life everywhere Planets, stars, galaxies, Big Bang Conception of size and distance Stars and the
More informationFIRST GRADE HAZARDS 1 WEEK LESSON PLANS AND ACTIVITIES
FIRST GRADE HAZARDS 1 WEEK LESSON PLANS AND ACTIVITIES PLATE TECTONIC CYCLE OVERVIEW OF FIRST GRADE VOLCANOES WEEK 1. PRE: Learning the shapes of volcanoes. LAB: Experimenting with "lava." POST: Comparing
More informationChapter 7: Volcanoes 8/18/2014. Section 1 (Volcanoes and Plate Tectonics) 8 th Grade. Ring of Fire
Section 1 (Volcanoes and Plate Tectonics) Chapter 7: Volcanoes 8 th Grade Ring of Fire a major belt of es that rims the Pacific Ocean Volcanic belts form along the boundaries of Earth s plates as they
More informationWhat do we know about Mars? Lesson Review
Name Class Date What do we know about Mars? Complete the following. 1. What gas makes up most of the atmosphere of Mars? 2. What do scientists think are the reasons that there is no liquid water on Mars
More informationMoon 101. Bellaire High School Team: Rachel Fisher, Clint Wu, Omkar Joshi
Moon 101 Bellaire High School Team: Rachel Fisher, Clint Wu, Omkar Joshi Part I Formation of the Moon Planetary Formation In the solar nebula, dust particles coalesced to form smaller planetesimals and
More informationThe 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 informationMSIP PROPOSAL TEAM OMICRON
MSIP PROPOSAL TEAM OMICRON QUESTION: How much more destructive is the lava flow from Olympus Mons compared to a smaller volcano like Biblis Patera? Centennial High School Peoria, AZ Question: How much
More informationUnit 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 informationChapter 9 Lecture. The Cosmic Perspective Seventh Edition. Planetary Geology: Earth and the Other Terrestrial Worlds Pearson Education, Inc.
Chapter 9 Lecture The Cosmic Perspective Seventh Edition Planetary Geology: Earth and the Other Terrestrial Worlds Planetary Geology: Earth and the Other Terrestrial Worlds 9.1 Connecting Planetary Interiors
More informationFor the next few weeks: Terrestrial Planets, their Moons, and the Sun. Planetary Surfaces and Interiors 2/20/07
For the next few weeks: Terrestrial Planets, their Moons, and the Sun Announcements Reading Assignment Section 9-1 (pp 186-189), 9-5 and 9-6 (pp 199-203) 3 rd Homework is now posted on the course website
More informationDistance 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 informationMars Update. Presented by NASA/JPL Solar System Educator Don W. Brown
Mars Update Presented by NASA/JPL Solar System Educator Don W. Brown http://www.wired.com/wiredscience/2010/01/gallery-mars/6/ Mariner Mars Climate Orbiter Mars Exploration Rovers Mars Global Surveyor
More informationMission to Mars! IS EARTH THE ONLY PLANET TO EXPERIENCE PLATE TECTONICS?
Mission to Mars! IS EARTH THE ONLY PLANET TO EXPERIENCE PLATE TECTONICS? PLATE TECTONICS Earth s crust is split up into several tectonic plates which are constantly moving around (about the same speed
More informationEffect of Albedo Change on Martian Temperature
Effect of Albedo Change on Martian Temperature Upper Darby High School, Period 5 Introduction: Similar to Earth, Mars is experiencing a period of global warming. However, the causes for global warming
More informationA first and last outpost for life on Mars? Insights from ancient hot springs in the Pilbara
A first and last outpost for life on Mars? Insights from ancient hot springs in the Pilbara What can studying early life on Earth tell us about origins of life? How can this shape our search for life elsewhere?
More informationImpact Cratering. David A. Hardy MARS EDUCATION PROGRAM
Impact Cratering David A. Hardy MARS EDUCATION PROGRAM Impact cratering overview: What we will learn about impact craters today: Causes of impacts - meteorites! Impact craters in our solar system Formation
More informationNASA The planets in our solar system are all different sizes.
Non-fiction: Explore Space Explore Space Our Solar System Our solar system is made up of the sun and eight planets. A planet is a large ball made of rock or gas. Each planet orbits, or travels around,
More information2018 Decimals 2. Name: EP 4/ #
2018 Decimals 2 Worksheet #1: Addition Worksheet #2: Subtraction Worksheet #3: Multiplication Worksheet #4: Division Worksheet #5: Estimation Worksheet #6: Word Problems Plus activities Name: EP 4/ # Addition
More informationA medium-sized star. The hottest object found in our solar system.
A medium-sized star. The hottest object found in our solar system. It gives off heat, light, and energy. It affects the seasons, climate, and weather on Earth. The second smallest planet in our solar system.
More informationTypes of Volcanoes. Key Concept: Tectonic plate motions can result in volcanic activity at plate boundaries.
Types of Volcanoes Key Concept: Tectonic plate motions can result in volcanic activity at plate boundaries. Volcanoes How do volcanoes work? How do volcanoes work? Magma is forced onto Earth s surface.
More informationTypes of Volcanoes KEY CONCEPT: TECTONIC PLATE MOTIONS CAN RESULT IN VOLCANIC ACTIVITY AT PLATE BOUNDARIES.
Types of Volcanoes KEY CONCEPT: TECTONIC PLATE MOTIONS CAN RESULT IN VOLCANIC ACTIVITY AT PLATE BOUNDARIES. Volcanoes How do volcanoes work? How do volcanoes work? Magma is forced onto Earth s surface.
More information