Planetary Geology pdf - NASA

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Figure 13.2. Photomosaic of Enceladus constructed from Voyager 2 images with resolutions of about 2 km/pixel. The satellite has a diameter of approximately 500 km. (Jet Propulsion Laboratory photomosaic P-23956 BW). Exercise Thirteen: The Geology of Outer Planet Satellites 163 EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences
A Figure 13.3. The surface of Rhea, seen by Voyager 1 at 700 m/pixel (FDS 34952.59). 164 B 50 km Exercise Thirteen: The Geology of Outer Planet Satellites 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
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e. Determine the sequence of events
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Exercise Three: Geologic Landforms
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Exercise Three: Geologic Landforms
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N Figure 3.8. Sierra Caballos Mount
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Exercise Four Impact Cratering Inst
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Objective To determine the initial
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Name Exercise Four Impact Cratering
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Sketch area In the fourth section o
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Part C Shot 1 (smallest) Shot 2 (ne
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10 km Exercise Four: Impact Crateri
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Science Standards ■ Earth and Spa
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Figure 5.1. Comparison of the forma
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Exercise Five Purpose To illustrate
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Part B: Volcanic Explosive Craterin
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N 100 km Figure 5.5. Olympus Mons,
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Exercise Six Suggested Correlation
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Figure 6.1. Different sand surfaces
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Exercise Six Purpose To learn how p
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*c. What geologic process(es) forme
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Figure 6.4. Photograph of lunar mar
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Exercise Seven Coriolis Effect Inst
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Purpose By tracing an object as it
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N 100 km Figure 7.1. Centered at 20
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elow this is the solid core of the
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for turbulent, inclement weather on
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7. Examine the atmosphere of Venus
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Figure 8.5. Viking Orbiter image 78
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N 102 Figure 8.7. Jupiter as seen b
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emove the flaps). Three windows are
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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
Page 145 and 146: 17. a. Volcanism. b. It shows a som
Page 147 and 148: Properties of the Major Satellites*
Page 149 and 150: The surface of Enceladus can be div
Page 151 and 152: . Describe in detail the shape of t
Page 153: Figure 13.1.b. Geological sketch ma
Page 157 and 158: Exercise Fourteen Planets in Stereo
Page 159 and 160: Exercise Fourteen: Planets in Stere
Page 161 and 162: 9. Examine the stereo images of Fig
Page 163 and 164: . Sketch what a profile across a ty
Page 165 and 166: 5 km Figure 14.3. Crater Geopert-Me
Page 167 and 168: Exercise Fourteen: Planets in Stere
Page 169 and 170: 25 km Figure 14.10. The icy uranian
Page 171 and 172: Exercise Fifteen Suggested Correlat
Page 173 and 174: Exercise Fifteen Purpose The object
Page 175 and 176: 3. What is the age relation between
Page 177 and 178: Figure 15.1. Sample geologic map an
Page 179 and 180: Figure 15.3. Apollo 15 photograph o
Page 181 and 182: Part A 1. Contacts are sharp; trans
Page 183 and 184: Geologic History Youngest Youngest
Page 185 and 186: Exercise Sixteen Purpose Through ob
Page 187 and 188: To establish age relations and inte
Page 189 and 190: Figure 16.1. Sample geologic map an
Page 191 and 192: Figure 16.3. Diagram of typical imp
Page 193 and 194: Exercise Sixteen: Photogeologic Map
Page 195 and 196: Figure 16.8. Northwest quadrant of
Page 197 and 198: Figure 16.10. Southeast quadrant of
Page 199 and 200: Youngest Youngest Oldest Oldest Fig
Page 201 and 202: Answer Key Map after 1) Scott et al
Page 203 and 204: Exercise Seventeen Purpose Through
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Figure 17.2. Sample geologic map an
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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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