Planetary Geology pdf - NASA

More documents

Recommendations

Info

Figure 14.1. Stereoscopic photographs of the Hadley Rille area of the Moon, landing site of Apollo 15. The sinuous trough (Hadley Rille) is about 300 m deep. The prominent crater, Hadley, is 5.7 km in diameter. North is toward the top. (Left half is part of AS15-0586, right half, AS15-0585. Spacecraft motion was from left to right parallel to the bottom edges of the photos). 174 Exercise Fourteen: Planets in Stereo Activities in Planetary Geology for the Physical and Earth Sciences EG-1998-03-109-HQ
5 km Figure 14.3. Crater Geopert-Meyer and surrounding features on Venus. The prominent trough is about 1 km deep, and the scene is about 154 km across. North is toward the top (NASA P-42612). Exercise Fourteen: Planets in Stereo N 175 Figure 14.2. Stereoscopic photographs of the Ares Vallis region of Mars, constructed from Viking orbiter images. North is toward the upper right. The prominent crater is about 7 km across. The Viking 1 Lander site is about 800 km to the west. (Viking Orbiter 004A52, left, and 004A93, right). 20 km EG-1998-03-109-HQ Activities in Planetary Geology for the Physical and Earth Sciences N
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 and 42:
. 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 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: . Sketch what a profile across a ty
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
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?