2 -- Formation of the Proto-Earth in the Solar Nebula2.1 EVOLUTION OF MOLECULAR CLOUDS TO THE SOLAR NEBULA; 2.2 FROM THE PRESOLAR NEBULA TO THE SOLAR SYSTEM; 2.3 AGE DATING BY RADIOACTIVE ISOTOPES; 2.4 MODEL AGE; 2.5 EXTINCT NUCLIDES; 2.6 THE 182HF-182W ISOTOPE SYSTEM; 2.7 MASS SPECTROMETRY; 2.7.1 Thermal Ionization Mass Spectrometry and Negative Thermal Ionization Mass Spectrometry; 2.7.2 Isotope Dilution Method; 2.7.3 Q-Pole Type Inductively Coupled Plasma Mass Spectrometry; 2.7.4 Multicollector Inductively Coupled Plasma Mass Spectrometry.
2.8 FORMATION OF GAS GIANT PLANETS AND ASTEROIDS: THE NICE MODEL2.9 THE LATE HEAVY BOMBARDMENT IN THE NICE MODEL; 2.10 THE GRAND TACK MODEL: THE RESONANCE OF JUPITER AND SATURN; 2.11 FORMATION OF INNER PLANETS IN THE GRAND TACK MODEL; 2.12 INCONSISTENCY BETWEEN OUR SOLAR SYSTEM AND EXOSOLAR SYSTEMS FOUND BY THE KEPLER PROGRAM; 2.13 OBSERVATION OF PLANETS AND ASTEROID BELTS; 2.13.1 The Planetary System; 2.13.2 Observation of the Asteroids; 2.13.3 Observation of the Asteroids From Space; 2.13.4 Sample Return Program From an Asteroid; References.
3 -- THE GIANT IMPACT MADE THE PRESENT EARTH1397059140MOON SYSTEM*3.1 INTRODUCTION; 3.2 HISTORY OF A GIANT IMPACT MODEL; 3.3 APOLLO PROGRAM: LANDING ON THE MOON AND SAMPLING MOON ROCKS; 3.3.1 The Apollo Program; 3.3.2 Rocks From the/ oon; 3.4 SIMILARITY BETWEEN CHEMICAL COMPOSITIONS OF THE MOON AND EARTH'S MANTLE; 3.5 CONSTRAINTS FROM HIGH FIELD STRENGTH ELEMENT; 3.6 MASS FRACTIONATION OF OXYGEN ISOTOPIC RATIO OF 18O/16O; 3.7 MASS FRACTIONATION OF THREE OXYGEN ISOTOPE RATIOS; 3.7.1 Definition of Three Oxygen Isotope Mass Fractionation; 3.7.2 Mass Fractionation Laws.
