Planetary Geology pdf - NASA

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15. List some similarities and differences between the landforms of the Earth and: a. Moon b. Mercury c. Mars d. Venus 16. Based on the number of craters, the number of geologic processes evident and the different types of landforms seen on the images, list the five surfaces you have examined in order : a. From oldest to youngest. b. From least complex to most complex. 17. Examine the table on the next page. Using a compass, draw circles showing the relative sizes of Mercury, Venus, Mars, the Moon, and Earth in the sketch area below. Let the diameter of Earth equal 6 cm. Sketch area Exercise Ten: Landform Mapping: The Terrestrial Planets EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences 119
Mercury Venus Earth Moon Mars Mean Distance from 384,400 km 57.9 108.2 149.6 Sun (millions of km) from Earth Equatorial Diameter (km) Equatorial Diameter (Earth diameters) Mass (relative to Earth) Volume (relative to Earth) 120 227.9 4880 12,104 12,756 3476 6787 0.38 0.95 1.000 0.272 0.53 0.055 0.815 1.000 0.0123 0.108 0.06 0.88 1.000 0.0203 0.15 Density (g/cm 3 ) 5.4 5.2 5.5 3.34 3.9 *18. Before the initial reconnaissance of the solar system by spacecraft was completed, it was traditionally believed that the geological complexity of surface features on a solar system body would be related to the size of the body, larger planets being more geologically complex. Is this true of the terrestrial planets? Support your answer. Exercise Ten: Landform Mapping: The Terrestrial Planets Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
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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
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 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
Page 111: 6. Based on the number of craters,
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 and 162: 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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