Preface |
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xi | |
Part I: Philosophical Aspects of Panspermia |
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1 | (52) |
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1 "On the Origin of Life" |
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3 | (4) |
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2 Why We Should Take Interstellar Panspermia Seriously |
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7 | (12) |
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7 | (1) |
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2.2 The Case for Interstellar Panspermia |
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8 | (3) |
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2.3 Theoretical Consequences of Interstellar Panspermia |
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11 | (3) |
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14 | (1) |
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15 | (4) |
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3 The Extended Continuity Thesis, Chronocentrism, and Directed Panspermia |
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19 | (22) |
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3.1 Introduction: The Continuity as a Pre-Requisite for Scientific Grounding of Astrobiology |
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20 | (2) |
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3.2 Versions and Resistance |
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22 | (4) |
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3.3 Cultural Evolution and Directed Panspermia |
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26 | (8) |
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3.4 Conclusion and Prospects |
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34 | (2) |
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36 | (1) |
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37 | (4) |
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4 Life in the Milky Way: The Panspermia Prospects |
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41 | (12) |
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41 | (2) |
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4.2 Three Levels of Habitability and Panspermia |
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43 | (5) |
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4.2.1 Stellar System Level |
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43 | (2) |
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4.2.2 Galaxies: Cosmic Cradles of Life |
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45 | (2) |
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4.2.3 Cosmological Level: Interactions of Galaxies |
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47 | (1) |
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48 | (1) |
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49 | (1) |
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49 | (4) |
Part II: Microorganisms and Panspermia |
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53 | (72) |
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5 Planetary Protection: Too Late |
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55 | (38) |
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56 | (1) |
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5.2 What is Planetary Protection |
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56 | (4) |
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5.3 Extent of Earth Biosphere |
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60 | (2) |
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5.4 Extension to Other Planetary Bodies |
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62 | (4) |
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62 | (2) |
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64 | (2) |
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66 | (1) |
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5.5 Backward Contamination |
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66 | (2) |
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5.6 Interplanetary Exchange |
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68 | (3) |
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5.7 Habitable Conditions for Interplanetary Micronauts |
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71 | (3) |
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74 | (3) |
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77 | (1) |
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78 | (1) |
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78 | (3) |
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81 | (1) |
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82 | (11) |
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6 Microbial Survival and Adaptation in Extreme Terrestrial Environments-The Case of the Dallol Geothermal Area in Ethiopia |
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93 | (26) |
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94 | (1) |
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6.2 Planetary Field Analog: The Case of the Dallol Geothermal Area |
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95 | (10) |
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6.2.1 The Dallol Hot Springs |
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99 | (5) |
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6.2.2 Dallol Geothermal Area Planetary Field Analogs |
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104 | (1) |
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6.3 Life in Extreme Environments |
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105 | (5) |
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6.4 Conclusion and Remarks on Panspermia |
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110 | (1) |
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111 | (1) |
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111 | (8) |
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7 Escape From Planet Earth: From Directed Panspermia to Terraformation |
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119 | (6) |
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123 | (1) |
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123 | (2) |
Part III: Formation and Evolution of Planets: Material Exchange Prospects |
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125 | (142) |
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8 Catalyzed Lithopanspermia Through Disk Capture of Biologically Active Interstellar Material |
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127 | (22) |
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128 | (1) |
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8.2 Capture of Interstellar Planetesimals |
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129 | (8) |
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8.2.1 Planetesimal Size Distribution |
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129 | (1) |
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130 | (1) |
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131 | (2) |
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8.2.4 Capture Probability |
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133 | (2) |
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8.2.5 Total Number of Captured Planetesimals |
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135 | (2) |
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8.3 Catalyzed Lithopanspermia |
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137 | (5) |
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8.3.1 Types of Panspermia |
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138 | (1) |
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8.3.2 Fraction of Life-Bearing Rocks |
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139 | (1) |
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140 | (2) |
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8.4 Conclusion and Discussion |
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142 | (1) |
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143 | (1) |
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144 | (5) |
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9 Lithopanspermia at the Center of Spiral Galaxies |
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149 | (22) |
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150 | (2) |
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9.2 The Kepler Transit Survey and the Distribution of Living Worlds |
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152 | (1) |
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9.3 XUV Hydrodynamic Escape and the Formation of Habitable Evaporated Cores |
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153 | (4) |
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9.3.1 Activity of Supermassive Black Holes |
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154 | (1) |
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9.3.2 Overabundance of HECs Driven by Quasar Illumination |
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155 | (2) |
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9.4 Frequency of Exchange in High Stellar Densities |
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157 | (5) |
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9.4.1 Ejection of Planetary Bodies on Intragalactic Scales |
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158 | (2) |
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9.4.2 Implications for Other Stellar Populations |
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160 | (2) |
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162 | (1) |
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163 | (1) |
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164 | (7) |
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171 | (24) |
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172 | (1) |
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10.2 Earth and Its Isotopic World: Geological and Environmental Implications |
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172 | (1) |
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10.3 Quest for the Primordial Water Worlds |
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173 | (3) |
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10.4 Looking for the Biotic Traces in Extraterrestrial Material |
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176 | (2) |
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10.5 Ices of the Moon and Proposal of Earth-Induced Wet Panspermia in the Solar System |
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178 | (4) |
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10.6 Implications for Other Planets of the Inner Solar System? |
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182 | (3) |
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185 | (1) |
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186 | (9) |
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11 There Were Plenty of Day/Night Cycles That Could Have Accelerated an Origin of Life on Earth, Without Requiring Panspermia |
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195 | (12) |
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202 | (1) |
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202 | (5) |
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12 Micrometeoroids as Carriers of Organics: Modeling of the Atmospheric Entry and Chemical Decomposition of Sub-Millimeter Grains |
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207 | (44) |
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12.1 Micrometeorites and the Search for Life |
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208 | (2) |
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210 | (4) |
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12.2.1 Carbonates in Space |
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211 | (2) |
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213 | (1) |
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12.3 Atmospheric Entry Model |
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214 | (5) |
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219 | (11) |
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12.4.1 Atmospheric Entry of MgCO3 Micrometeoroids |
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220 | (3) |
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12.4.2 Atmospheric Entry of CaCO3 Micrometeoroids |
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223 | (3) |
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12.4.3 Atmospheric Entry of FeCO3 Micrometeoroids |
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226 | (3) |
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12.4.4 Atmospheric Entry of CaSO4 Micrometeoroids |
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229 | (1) |
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12.5 The Role of Primordial Atmospheres |
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230 | (11) |
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12.5.1 Isothermal Atmosphere Model |
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233 | (4) |
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12.5.2 Hydrogen Atmosphere |
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237 | (2) |
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12.5.3 Carbon Dioxide Atmosphere |
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239 | (1) |
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12.5.4 Methane Atmosphere |
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239 | (2) |
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241 | (2) |
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243 | (8) |
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13 Dynamical Evolution of Planetary Systems: Role of Planetesimals |
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251 | (16) |
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251 | (2) |
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13.2 Planetesimal Formation and Evolution |
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253 | (2) |
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13.3 Transporting Mechanism in Later Stages of Planetary System Evolution |
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255 | (6) |
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261 | (1) |
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262 | (1) |
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262 | (5) |
Part IV: Further Prospects |
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267 | (60) |
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14 A Survey of Solar System and Galactic Objects With Pristine Surfaces That Record History and Perhaps Panspermia, With a Plan for Exploration |
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269 | (40) |
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269 | (10) |
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270 | (1) |
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271 | (1) |
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14.1.2.1 Supernovae and Gamma-Ray Bursts |
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272 | (1) |
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272 | (1) |
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14.1.2.3 Background Radiation From Galactic Sources |
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273 | (1) |
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273 | (2) |
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275 | (4) |
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14.2 Recording Properties |
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279 | (2) |
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14.3 Pristine Potential of Solar System Bodies |
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281 | (7) |
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14.3.1 Comets, Asteroids and Dwarf Planets |
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281 | (2) |
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283 | (1) |
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283 | (1) |
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283 | (1) |
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14.3.5 Main Asteroid Belt |
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284 | (1) |
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14.3.6 Jupiter and Saturn |
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285 | (1) |
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14.3.7 Uranus and Neptune |
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286 | (1) |
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286 | (1) |
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287 | (1) |
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287 | (1) |
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14.3.11 Extra-Solar Bodies |
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288 | (1) |
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14.4 Prospects and Conclusions |
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288 | (1) |
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289 | (1) |
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289 | (20) |
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15 The Panspermia Publications of Sir Fred Hoyle |
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309 | (18) |
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316 | (1) |
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316 | (11) |
Index |
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327 | |