Planetary Geology pdf - NASA

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Part D. Asteroid Ida. A stereoscopic view of asteroid 243 Ida is shown in Figure 14.6. 12. Compare the overall shape of Ida to that of other planetary bodies you have studied. What is unusual about the asteroidÕs shape? 13. What geological process has affected the surface of Ida? How might this process account for the asteroidÕs overall shape? Part E. Outer Planet Satellites. The following figures show stereoscopic images of some of the satellites of Saturn and Uranus. Only five satellites are shown, a sampling of the dozens of moons of the outer planets. All of the moons shown have icerich surfaces, and none have atmospheres. Figures 14.7 and 14.8 show Rhea and Dione, respectively. These are two of SaturnÕs icy satellites. 14. What geologic process has most shaped the surface of Rhea? 15. Compare the appearance of craters on Dione to those on Rhea. Include both similarities and differences in their morphologies. 16. a. Which satellite appears to have an older surface, Rhea or Dione? How can you tell? b. What does this say about whether these satellites might have been resurfaced by volcanism at some time in the past? Figures 14.9, 14.10, and 14.11 show Titania, Ariel, and Miranda, respectively. These are icy satellites of planet Uranus. 17. Notice the prominent feature that stretches across the surface of Titania (Figure 14.9). a. Describe this feature. b. What process is responsible for its formation? 18. Several valleys cross the surface of Ariel , especially near the terminator (the day/night line), visible on the right side of the stereo image (Figure 14.10). a. What is unusual about the appearance of the material in these valleys? 172 Exercise Fourteen: Planets in Stereo Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
. Sketch what a profile across a typical one of these valleys might look like in the sketch area below. Sketch area c. What two processes probably acted together to form these features? 19. The surface of Miranda (Figure 14.11) consists of cratered terrain and several regions termed ÒcoronaeÓ (singular: corona). In contrast to the cratered terrain, the coronae consist of light and dark materials. a. Describe the topography and character of the coronae as compared to the cratered terrain which surrounds them. b. What process(es) have likely shaped the coronae of Miranda? Exercise Fourteen: Planets in Stereo 173 EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences
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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
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10. Based on your three sketches of
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The wind is at work on other planet
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Unit Four The three decades from th
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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 and 154: Figure 13.1.b. Geological sketch ma
Page 155 and 156: A Figure 13.3. The surface of Rhea,
Page 157 and 158: Exercise Fourteen Planets in Stereo
Page 159 and 160: Exercise Fourteen: Planets in Stere
Page 161: 9. Examine the stereo images of Fig
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 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
Page 207 and 208: Geologic History: Youngest Oldest E
Page 209 and 210: Erosion: Process whereby materials
Page 211 and 212: 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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