Planetary Geology pdf - NASA

More documents

Recommendations

Info

e. Sketch a non-exaggerated profile across Meteor Crater in the space below. Use a scale of 1cm = 200m. The present depth of the crater is about 85% of its original depth, due to erosional infilling. Use your answer from 5.b. to determine the present depth to use for your profile. Sketch area f. List some similarities and differences in the morphology of Meteor Crater compared to the volcanic summit crater seen in Figure 3.3. Synthesis Planetary surfaces represent combinations of some or all of the four geologic processes. In the following questions, you will synthesize information from the previous questions and photographs. 6. Examine Figure 3.8, which shows the Caballos mountains of southwestern New Mexico. The two nearly featureless ÒislandsÓ of high standing rock are volcanic in origin. Beneath them are rocks that were laid down as sedimentary strata. a. Examine the strata of Figure 3.8, comparing this scene to Figures 3.5 and 3.6. Are the strata of the Caballos mountains tilted or flat-lying? b. Estimate the strike and dip directions of the strata in the region beneath the western ÒislandÓ of volcanic rock. c. What is the most likely explanation to account for the isolated islands of volcanic plains? d. Why are no impact craters visible in this area? 40 Exercise Three: Geologic Landforms Seen on Stereoscopic Photos Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
e. Determine the sequence of events that affected this region by numbering the events below from 1 (first event) to 4 (most recent event). Mark with an ÒxÓ the one event that did not occur in this region. ___ Tectonic forces caused folding and tilting of the rocks. ___ Sedimentary strata were laid down horizontally. ___ Volcanic plains were faulted and tilted. ___ Erosion by rivers and streams dissected the region. ___ Volcanic plains were laid down horizontally. Exercise Three: Geologic Landforms Seen on Stereoscopic Photos EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences 41
Page 1 and 2: National Aeronautics and Space Admi
Page 3 and 4: A ctivities in Planetary Geology fo
Page 5 and 6: Preface Introduction Special Note t
Page 7 and 8: 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: . Examine the broad, steep face tha
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 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 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 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:
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 205 and 206:
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
Page 213 and 214:
Cattermole, P. (1994). Venus: The G
Page 215 and 216:
Object Moon Moon Moon Moon Moon Moo
Page 217 and 218:
Object Jupiter Jupiter Jupiter Jupi
Page 219 and 220:
1.6 Regional Planetary Image Facili
Page 221 and 222:
2. Map Link 25 Eat Mason Santa Barb
Page 223:
NATIONAL AERONAUTICS AND SPACE ADMI
show all

Planetary Geology pdf - NASA

Create successful ePaper yourself

Delete template?

Save as template?