Introduction to Planetary Science

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$P 0.1 Stabilişti natura şsi suma seriilor: a) Σ 1 n\ ; b) Σ arctan 1 n# + n ...$

86 chapter 6 Schopf JW (ed) Earth’s Earliest Biosphere: Its Origin and Evolution. Princeton University Press, Princeton, NJ, pp. 32–40 Taylor SR (1992) Solar system evolution: A new perspective. Cambridge University Press, New York Van Allen JA, Bagenal F (1999) Planetary magnetospheres and the interplanetary medium. In: Beatty JK, Petersen CC, Chaikin A. (eds) The New Solar System, 39–58, 4th edn. Sky Publishing Corp., Cambridge, MA Valley JW (2005) A cool early Earth? Sci Am 293:57–65 Wagner JK (1991) Introduction to the solar system. Saunders College Pub., Orlando, Florida Wilde SA, Valley JW, Peck YH, Graham CM (2001) Evidence from detrital zircons for the existence of continental crust and oceans on the Earth 4.4 billion years ago. Nature 409:175–178 Wilson M (1989) Igneous petrogenesis: A global tectonic approach. Unwin Hyman, London, UK Wyllie PJ (1971) The dynamic Earth: Textbook in geosciences. Wiley, New York
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Introduction to Planetary Science
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A C.I.P. Catalogue record for this
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Table of Contents Preface xvii 1. T
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table of contents ix 7.3.4. The Ear
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table of contents xi 12.1.2. Physic
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table of contents xiii 15.6. Scienc
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table of contents xv 22.8. Summary
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Preface This textbook is intended t
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preface xix structure, their geolog
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On May 25, 1961, President John F.
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the urge to explore 3 deliberating
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the urge to explore 5 not catch on,
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the urge to explore 7 Figure 1.4. W
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the urge to explore 9 After a space
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the urge to explore 11 1.5.3 Averag
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Since time beyond reckoning, humans
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from speculation to understanding 1
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24 chapter 3 International Astronom
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26 chapter 3 Table 3.2. Average rad
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28 chapter 3 3.4 Surface Temperatur
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30 chapter 3 Figure 3.5. The densit
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32 chapter 3 core, which is presume
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34 chapter 3 3.8 Problems 1. Calcul
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36 chapter 4 Table 4.1. Types of ma
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38 chapter 4 Table 4.2. The basic c
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40 chapter 4 Figure 4.3. The Hertzs
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42 chapter 4 The unstable nucleus o
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44 chapter 4 in their central bulge
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46 chapter 4 About 10 −43 seconds
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48 chapter 4 3. Calculate the age o
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50 chapter 5 Table 5.1. The periodi
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52 chapter 5 The contraction of the
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54 chapter 5 Figure 5.2. The interi
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56 chapter 5 5.3.2 Energy Productio
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58 chapter 5 to the axis of rotatio
Page 154: 60 chapter 5 Figure 5.8. The solar
Page 158: 62 chapter 5 the radii of their orb
Page 162: The Earth in Figure 6.1 is the most
Page 166: earth: model of planetary evolution
Page 208: 88 chapter 7 his own work demonstra
Page 212: 90 chapter 7 Figure 7.2. According
Page 216: 92 chapter 7 Figure 7.3. The orbita
Page 220: 94 chapter 7 Figure 7.5. The inferi
Page 224: 96 chapter 7 Figure 7.6. The synodi
Page 228: 98 chapter 7 Nothing in our every-d
Page 232: 100 chapter 7 Figure 7.9. The gravi
Page 236: 102 chapter 7 Figure 7.11. The seas
Page 240: 104 chapter 7 Figure 7.13. Variatio
Page 244: 106 chapter 7 7.6.3 Synodic Periods
Page 248: 108 chapter 7 Clark GR II (1968) Mo
Page 252: 110 chapter 8 Figure 8.1. Ahnighito
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112 chapter 8 Figure 8.2. The Sikho
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114 chapter 8 Figure 8.4. A. Allend
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116 chapter 8 fragments of still la
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118 chapter 8 Figure 8.8. The numbe
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120 chapter 8 continents without a
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122 chapter 8 Table 8.3. Elements t
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124 chapter 8 Figure 8.11. The stru
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126 chapter 8 the present rate. Nev
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128 chapter 8 Figure 8.15. Devastat
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130 chapter 8 time. As a result, a
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132 chapter 8 P 0 = number of paren
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134 chapter 8 where the radius r =
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136 chapter 8 Dietz RS (1947) Meteo
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The Moon in Figure 9.1 is the only
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the earth-moon system 141 Figure 9.
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the earth-moon system 143 3. Erupti
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the earth-moon system 149 Table 9.2
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the earth-moon system 151 one trill
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the earth-moon system 153 crystalli
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the earth-moon system 155 Moon does
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the earth-moon system 159 e. Explor
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the earth-moon system 163 9.12 Scie
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the earth-moon system 165 desired n
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Mercury is the smallest of the terr
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mercury: too hot for comfort 169 Th
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mercury: too hot for comfort 171 te
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mercury: too hot for comfort 173 Fi
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mercury: too hot for comfort 177 of
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mercury: too hot for comfort 181 a
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184 chapter 11 Figure 11.1. The fou
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186 chapter 11 Figure 11.3. Shaded
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188 chapter 11 Figure 11.5. Lava fl
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190 chapter 11 Figure 11.7. Lava do
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192 chapter 11 Table 11.1. Chemical
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194 chapter 11 Figure 11.11. Illust
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196 chapter 11 Figure 11.13. A set
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198 chapter 11 Figure 11.15. Most o
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200 chapter 11 Figure 11.16. The ca
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202 chapter 11 An alternative expla
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204 chapter 11 The problem with thi
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206 chapter 11 atmospheric pressure
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208 chapter 11 radiation and theref
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210 chapter 11 Nimmo F, McKenzie D
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212 chapter 12 Figure 12.1. This gl
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214 chapter 12 decompression meltin
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216 chapter 12 Table 12.3. Orbital
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218 chapter 12 northern hemisphere
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220 chapter 12 lava flows on the su
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222 chapter 12 Figure 12.5. Aerial
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224 chapter 12 Figure 12.7. The lan
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226 chapter 12 Figure 12.8. The sur
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228 chapter 12 12.4.3 Hadriaca Pate
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230 chapter 12 a gradual decrease o
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232 chapter 12 Figure 12.13. Yuty c
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234 chapter 12 Figure 12.14. The su
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236 chapter 12 The effectiveness of
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238 chapter 12 capable of drilling
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240 chapter 12 Figure 12.18. Topogr
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242 chapter 12 hundred million year
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244 chapter 12 Figure 12.19. Sawed
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246 chapter 12 January 3, 2004. Thi
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248 chapter 12 Figure 12.23. The ro
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250 chapter 12 life-support systems
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252 chapter 12 being tested by NASA
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254 chapter 12 consisting of the ox
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256 chapter 12 in the hot deserts o
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258 chapter 12 pressure. When the f
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The solar system contains hundreds
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asteroids: shattered worlds 263 Tab
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asteroids: shattered worlds 265 Fig
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asteroids: shattered worlds 267 Onl
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asteroids: shattered worlds 269 cra
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asteroids: shattered worlds 271 Fig
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asteroids: shattered worlds 273 13.
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asteroids: shattered worlds 275 yea
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asteroids: shattered worlds 277 the
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asteroids: shattered worlds 279 3 Y
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We now enter the outer regions of t
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jupiter: heavy-weight champion 283
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298 chapter 15 Figure 15.1. The mon
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300 chapter 15 distance from the ce
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302 chapter 15 surprisingly short a
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304 chapter 15 fields were not stro
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306 chapter 15 Table 15.2. Major vo
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308 chapter 15 insulates the hot la
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310 chapter 15 Figure 15.9. Complex
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312 chapter 15 appears to be circul
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314 chapter 15 to 2.38 km/s for the
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316 chapter 15 ice remain on opposi
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318 chapter 15 Table 15.3. Impact c
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320 chapter 15 of explaining the fo
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322 chapter 15 where life did origi
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324 chapter 15 Figure 15.16. Ganyme
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326 chapter 15 Figure 15.18. Close-
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328 chapter 15 two times longer tha
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330 chapter 15 Figure 15.21. The As
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332 chapter 15 Substituting into eq
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Saturn in Figure 16.1 is the second
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saturn: the beauty of rings 337 Tab
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saturn: the beauty of rings 339 (0.
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saturn: the beauty of rings 341 and
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saturn: the beauty of rings 343 mos
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saturn: the beauty of rings 345 Fig
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saturn: the beauty of rings 347 Fig
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saturn: the beauty of rings 349 mol
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saturn: the beauty of rings 351 16.
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saturn: the beauty of rings 353 3.
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saturn: the beauty of rings 355 met
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saturn: the beauty of rings 357 Mor
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360 chapter 17 Figure 17.1. The sur
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362 chapter 17 constituent within a
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364 chapter 17 resulted from the de
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366 chapter 17 overheating of the E
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The planet Uranus in Figure 18.1 wa
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uranus: what happened here? 371 Tab
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uranus: what happened here? 373 to
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uranus: what happened here? 375 an
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uranus: what happened here? 377 the
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uranus: what happened here? 379 hav
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uranus: what happened here? 381 Fig
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uranus: what happened here? 383 Not
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After Uranus had been discovered in
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neptune: more surprises 387 Triton
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neptune: more surprises 389 about 2
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neptune: more surprises 391 electri
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neptune: more surprises 393 its low
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neptune: more surprises 395 Figure
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neptune: more surprises 397 that Ne
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neptune: more surprises 399 Encyclo
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402 chapter 20 Figure 20.1. Pluto a
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404 chapter 20 Figure 20.2. The pla
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406 chapter 20 Figure 20.3. Pluto a
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408 chapter 20 Lang KR, Whitney CA
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410 chapter 21 The shapes and sizes
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412 chapter 21 Figure 21.2. The orb
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414 chapter 21 Figure 21.3. A. The
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416 chapter 21 approximately equal
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418 chapter 21 EKOs whose semi-majo
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Comets have played an important rol
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comets: coming inside from the cold
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Now that we have explored the plane
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earth: the cradle of humans 443 The
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earth: the cradle of humans 445 on
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earth: the cradle of humans 447 Fig
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earth: the cradle of humans 449 23.
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earth: the cradle of humans 451 sur
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earth: the cradle of humans 453 M.H
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456 chapter 24 A similar phenomenon
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458 chapter 24 object identified as
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460 chapter 24 of the Sun (i.e., 0.
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462 chapter 24 1. The distance of t
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464 chapter 24 television came into
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466 chapter 24 and to have a core t
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468 chapter 24 Tarter JC, Chyba CF
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470 appendix 1 A1.4.1 Distance (m)
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472 appendix 1 A1.14 Roche Limits T
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474 appendix 1 k = 138 × 10 −23
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476 appendix 2 (Continued) Planet S
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478 appendix 2 (Continued) Name a A
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Glossary Geographic places and the
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glossary 483 Biosphere The total of
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glossary 485 Dormant volcano A volc
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glossary 487 Gas tail The part of t
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glossary 489 Intelligence The chara
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glossary 491 Main-belt asteroids As
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glossary 493 Nuclear fission A reac
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glossary 495 Pioneer American progr
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glossary 497 Red shift The increase
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glossary 499 Snowball Earth A somew
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glossary 501 Tidal forces The diffe
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Only the names of the first authors
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author index 505 Graedel, T.E. 101,
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author index 507 P Papanastassiou,
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d = diagram, t = table, p = photogr
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subject index 511 Celetial mechanic
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subject index 513 physical properti
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subject index 515 Hydrogen fusion r
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subject index 517 Gusev crater 246-
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subject index 519 kinetic energy, T
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subject index 521 Nuclear weapons,
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subject index 523 Solar system dwar
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subject index 525 basalt 187-192, 1
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