Planetary Geology pdf - NASA

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Figure 8.4. Earth as seen from the Geostationary Operational Environmental Satellite, GOES-7. The picture was taken at 6 p.m. Greenwich Mean Time on September 25, 1994, soon after the start of northern hemisphere autumn. The north pole is toward the top. Exercise Eight: Storm Systems EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences 99
Figure 8.5. Viking Orbiter image 78A42, showing a water frost cloud pattern over the surface of Mars. North is toward the top. 100 Exercise Eight: Storm Systems Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ N
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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
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Exercise One Suggested Correlation
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Part One 1. (Answers will vary.) Vo
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5. Based on the number of pictures
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_____ 08/19/92 earthquake, central
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165° W 75°W 0° 75°E180°E 75°N
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1. a. The volcano has a circular ba
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Exercise Two Volcanism Purpose By s
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7. List some factors that might aff
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. How is it similar? Examine the vi
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N 200 m Figure 2.1. Mount Capulin,
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N Figure 2.3. Oblique aerial view o
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Figures 2.7.a., 2.7.b. Meteor Crate
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N Figure 2.9. Mosaic of Landsat fra
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1. a. Sketch should show steep side
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Exercise Three Purpose By using ste
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Gradation 2. Figure 3.4 shows a por
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. 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 and 60: Part C Shot 1 (smallest) Shot 2 (ne
Page 61 and 62: 10 km Exercise Four: Impact Crateri
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: 7. Examine the atmosphere of Venus
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
Page 111 and 112: 6. Based on the number of craters,
Page 113 and 114: Mercury Venus Earth Moon Mars Mean
Page 115 and 116: Figure 10.2. Mariner 10 mosaic of M
Page 117 and 118: C Figure 10.4. Magellan radar mosai
Page 119 and 120: Exercise Eleven Suggested Correlati
Page 121 and 122: Exercise Eleven Purpose To learn to
Page 123 and 124: . If windstreaks are dust deposits
Page 125 and 126: Figure 11.2. Ius Chasma, part of th
Page 127 and 128: Exercise Eleven: Geologic Features
Page 129 and 130: Exercise Twelve Suggested Correlati
Page 131 and 132: Exercise Twelve Purpose To learn ab
Page 133 and 134: So far all the figures have shown f
Page 135 and 136: Figure 12.3. The prominent circular
Page 137 and 138: N 100 km Figure 12.6. Volcanoes com
Page 139 and 140: Exercise Twelve: Geologic Features
Page 141 and 142: Exercise Thirteen Suggested Correla
Page 143 and 144: 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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