Preface | p. xi |
Introduction | p. 1 |
Past Thinking about Earth-Like Planets and Life | p. 3 |
The Habitable Zone and the Importance of Liquid Water | p. 5 |
Carl Sagan and the Drake Equation | p. 9 |
Other Perspectives on Planetary Habitability: Rare Earth and Gaia | p. 11 |
Our Habitable Planet Earth | p. 15 |
Critical Updates on How Planets Are Built | p. 17 |
The Conventional Wisdom regarding Planet Formation | p. 18 |
Where Did Earth's Water Come From? | p. 21 |
New Models for Planetary Accretion and Delivery of Water | p. 23 |
Could Earth's Water Have Come from Comets? | p. 25 |
An Up-to-Date Simulation of Planetary Accretion | p. 28 |
Long-Term Climate Stability | p. 32 |
Solar Evolution Theory | p. 32 |
Solar Mass Loss? | p. 36 |
Electromagnetic Radiation and the Greenhouse Effect | p. 37 |
Planetary Energy Balance | p. 41 |
The Faint Young Sun Problem | p. 42 |
Possible Solutions to the Problem | p. 45 |
The Carbonate-Silicate Cycle and Controls on Atmospheric CO2 | p. 49 |
The CO2-Climate Feedback Loop | p. 53 |
More Wrinkles in Earths Climate History | p. 57 |
The Phanerozoic Climate Record | p. 58 |
Precambrian Climate | p. 63 |
Geologic Evidence for the Rise of Atmospheric O2 | p. 65 |
Cause of the O2 Rise: Cyanobacteria | p. 68 |
Methane, Methanogens, and the Universal Tree of Life | p. 71 |
The Archean Methane Greenhouse | p. 75 |
The Paleoproterozoic Glaciation | p. 77 |
Runaway Glaciation and "Snowball Earth" | p. 80 |
Milankovitch Cycles and the Recent Ice Ages | p. 81 |
Ice Albedo Feedback and Climatic Instability | p. 86 |
Evidence for Low-Latitude Glaciation | p. 88 |
Mechanisms for Explaining Low-Latitude Glaciation | p. 90 |
Snowball Earth | p. 92 |
Limits to Planetary Habitability | p. 97 |
Runaway Greenhouses and the Evolution of Venus' Atmosphere | p. 99 |
The History of Water on Venus | p. 100 |
The Classical Runaway Greenhouse Effect | p. 103 |
An Alternative Runaway Greenhouse Model | p. 106 |
Evolution of Venus' Atmosphere | p. 111 |
The Future Evolution of Earth | p. 116 |
High-CO2 Atmospheres and Temperature Limits for Life | p. 116 |
Future Solar Evolution and Lifetime of the Biosphere | p. 118 |
A Geoengineering Solution to Solar Luminosity Increases | p. 121 |
The Martian Climate Puzzle | p. 125 |
Evidence for Liquid Water near Mars' Surface | p. 126 |
CH4 in Mars' Atmosphere? | p. 130 |
Evidence That Water Flowed in Mars' Distant Past | p. 131 |
When Did the Martian Valleys Form? | p. 135 |
How Warm Was Early Mars? | p. 136 |
Mechanisms for Warming Early Mars | p. 138 |
Where Are the Carbonates? | p. 144 |
Is the Earth Rare? | p. 147 |
Planetary Size / Magnetic Fields | p. 147 |
Ozone and Ultraviolet Radiation | p. 152 |
Availability of Nitrogen and the Importance of N2 | p. 155 |
Is Plate Tectonics Common? | p. 157 |
A Planets Impact Environment | p. 161 |
Stabilization of Earth's Obliquity by the Moon | p. 164 |
Habitable Zones around Stars | p. 171 |
Historical Attempts to Define the Habitable Zone | p. 171 |
A More Modern Model for the Habitable Zone around the Sun | p. 176 |
Hertzsprung-Russell Diagrams and Main Sequence Stars | p. 179 |
Habitable Zones around Other Stars | p. 181 |
Problems for Planets Orbiting Early-Type Stars | p. 185 |
Problems for Planets Orbiting Late-Type Stars | p. 188 |
Further Extensions of the Habitable Zone Concept | p. 191 |
The Galactic Habitable Zone | p. 192 |
How to Find Another Earth | p. 195 |
Indirect Detection of Planets around Other Stars | p. 197 |
Barnard's Star | p. 198 |
The Astrometric Method | p. 199 |
Pulsar Planets | p. 205 |
The Doppler Effect | p. 207 |
The Radial Velocity Method | p. 210 |
Gravitational Microlensing | p. 216 |
Finding and Characterizing Planets by Using Transits | p. 221 |
Transits of Mercury and Venus | p. 221 |
Transits of Extrasolar "Hot Jupiters" | p. 222 |
Space-Based Transit Searches: CoRoT and Kepler | p. 227 |
Observing Exoplanet Atmospheres during Transits | p. 229 |
Secondary Transit Spectroscopy | p. 233 |
Characterizing Earth-Like Planets around M Stars | p. 235 |
Direct Detection of Extrasolar Planets | p. 239 |
What Wavelength Region Should We Choose? | p. 240 |
Infrared Interferometers: TPF-I and Darwin | p. 245 |
Searching for Planets at Visible Wavelengths: TPF-C | p. 248 |
The Visible Occulter: TPF-O | p. 253 |
Nearby Target Stars | p. 254 |
The Spectroscopic Search for Life | p. 258 |
Spectral Resolution | p. 259 |
The Visible/Near-IR Region: TPF-C or -O | p. 260 |
The Thermal-IR Region: TPF-I or Darwin | p. 266 |
Looking for Life on Early Earth-Type Planets | p. 269 |
Possible False Positives for Life | p. 271 |
Polarization Measurements: Looking for the Glint of Surface Water | p. 274 |
The Holy Grail: Simultaneous Detection of O2 and Reduced Gases | p. 276 |
Prospects for the More Distant Future | p. 284 |
NASA's Life Finder Mission | p. 284 |
Using the Sun as a Gravitational Lens | p. 287 |
The Drake Equation Revisited: The Search for Extraterrestrial Intelligence | p. 290 |
Notes | p. 299 |
Index | p. 317 |
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