Planetary Geology pdf - NASA

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*Part E d. How does the size of the projectile relate to crater size? e. Which is the most important factor controlling the crater size; the size, mass, or velocity of the projectile? Remove all projectiles from the sand tray and smooth the target surface. Divide the sand into two equal halves. In one half form a ridge of sand about 10 cm high and 15 cm wide, and leave the other half smooth. Use intermediate size steel ball bearings and form one crater on the side of the ridge. Form another crater on the flat section, launching it with the slingshot from 70 to 90 cm above the tray. Compare the two craters. *6. What can you say about crater preservation on rugged terrain versus smooth terrain? 60 Exercise Four: Impact Cratering Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
10 km Exercise Four: Impact Cratering N Figure 4.1. Apollo 15 photograph of lunar craters Messier A and B. The small crosses are camera registration marks. North is to the upper right corner of the photo. The oblong crater (Messier A) is 11 kilometers in diameter. (Apollo Metric frame AS152674). EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences 61
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National Aeronautics and Space Admi
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A ctivities in Planetary Geology fo
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Preface Introduction Special Note t
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We are living in a time of revoluti
Page 9 and 10: Exercise One Suggested Correlation
Page 11 and 12: Part One 1. (Answers will vary.) Vo
Page 13 and 14: 5. Based on the number of pictures
Page 15 and 16: _____ 08/19/92 earthquake, central
Page 17 and 18: 165° W 75°W 0° 75°E180°E 75°N
Page 19 and 20: 1. a. The volcano has a circular ba
Page 21 and 22: Exercise Two Volcanism Purpose By s
Page 23 and 24: 7. List some factors that might aff
Page 25 and 26: . How is it similar? Examine the vi
Page 27 and 28: N 200 m Figure 2.1. Mount Capulin,
Page 29 and 30: N Figure 2.3. Oblique aerial view o
Page 31 and 32: Figures 2.7.a., 2.7.b. Meteor Crate
Page 33 and 34: N Figure 2.9. Mosaic of Landsat fra
Page 35 and 36: 1. a. Sketch should show steep side
Page 37 and 38: Exercise Three Purpose By using ste
Page 39 and 40: Gradation 2. Figure 3.4 shows a por
Page 41 and 42: . Examine the broad, steep face tha
Page 43 and 44: e. Determine the sequence of events
Page 45 and 46: Exercise Three: Geologic Landforms
Page 47 and 48: Exercise Three: Geologic Landforms
Page 49 and 50: N Figure 3.8. Sierra Caballos Mount
Page 51 and 52: Exercise Four Impact Cratering Inst
Page 53 and 54: Objective To determine the initial
Page 55 and 56: Name Exercise Four Impact Cratering
Page 57 and 58: Sketch area In the fourth section o
Page 59: Part C Shot 1 (smallest) Shot 2 (ne
Page 63 and 64: Science Standards ■ Earth and Spa
Page 65 and 66: Figure 5.1. Comparison of the forma
Page 67 and 68: Exercise Five Purpose To illustrate
Page 69 and 70: Part B: Volcanic Explosive Craterin
Page 71 and 72: N 100 km Figure 5.5. Olympus Mons,
Page 73 and 74: Exercise Six Suggested Correlation
Page 75 and 76: Figure 6.1. Different sand surfaces
Page 77 and 78: Exercise Six Purpose To learn how p
Page 79 and 80: *c. What geologic process(es) forme
Page 81 and 82: Figure 6.4. Photograph of lunar mar
Page 83 and 84: Exercise Seven Coriolis Effect Inst
Page 85 and 86: Purpose By tracing an object as it
Page 87 and 88: N 100 km Figure 7.1. Centered at 20
Page 89 and 90: elow this is the solid core of the
Page 91 and 92: for turbulent, inclement weather on
Page 93 and 94: 7. Examine the atmosphere of Venus
Page 95 and 96: Figure 8.5. Viking Orbiter image 78
Page 97 and 98: N 102 Figure 8.7. Jupiter as seen b
Page 99 and 100: emove the flaps). Three windows are
Page 101 and 102: Purpose In this experiment you will
Page 103 and 104: 10. Based on your three sketches of
Page 105 and 106: The wind is at work on other planet
Page 107 and 108: Unit Four The three decades from th
Page 109 and 110: 1. The highlands are bright, rugged
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6. Based on the number of craters,
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Mercury Venus Earth Moon Mars Mean
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Figure 10.2. Mariner 10 mosaic of M
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C Figure 10.4. Magellan radar mosai
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Exercise Eleven Suggested Correlati
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Exercise Eleven Purpose To learn to
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. If windstreaks are dust deposits
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Figure 11.2. Ius Chasma, part of th
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Exercise Eleven: Geologic Features
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Exercise Twelve Suggested Correlati
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Exercise Twelve Purpose To learn ab
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So far all the figures have shown f
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Figure 12.3. The prominent circular
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N 100 km Figure 12.6. Volcanoes com
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Exercise Twelve: Geologic Features
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Exercise Thirteen Suggested Correla
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I. Ganymede 1. Ganymede orbits the
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17. a. Volcanism. b. It shows a som
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Properties of the Major Satellites*
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The surface of Enceladus can be div
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. Describe in detail the shape of t
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Figure 13.1.b. Geological sketch ma
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A Figure 13.3. The surface of Rhea,
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Exercise Fourteen Planets in Stereo
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Exercise Fourteen: Planets in Stere
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9. Examine the stereo images of Fig
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. Sketch what a profile across a ty
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5 km Figure 14.3. Crater Geopert-Me
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Exercise Fourteen: Planets in Stere
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25 km Figure 14.10. The icy uranian
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Exercise Fifteen Suggested Correlat
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Exercise Fifteen Purpose The object
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3. What is the age relation between
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Figure 15.1. Sample geologic map an
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Figure 15.3. Apollo 15 photograph o
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Part A 1. Contacts are sharp; trans
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Geologic History Youngest Youngest
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Exercise Sixteen Purpose Through ob
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To establish age relations and inte
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Figure 16.3. Diagram of typical imp
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Exercise Sixteen: Photogeologic Map
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Figure 16.8. Northwest quadrant of
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Figure 16.10. Southeast quadrant of
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Youngest Youngest Oldest Oldest Fig
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Answer Key Map after 1) Scott et al
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Exercise Seventeen Purpose Through
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Geologic History: Youngest Oldest E
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Erosion: Process whereby materials
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Terrain: A region of a surface shar
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Cattermole, P. (1994). Venus: The G
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Object Moon Moon Moon Moon Moon Moo
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Object Jupiter Jupiter Jupiter Jupi
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1.6 Regional Planetary Image Facili
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2. Map Link 25 Eat Mason Santa Barb
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NATIONAL AERONAUTICS AND SPACE ADMI
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