Planetary Formation, Geologic Time, and Earth's Core Composition
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Planetary Origins and Earth's Structure
1.1 The Formation of Earth
Our solar system was formed from a solar nebula, or cloud of gas and dust, that collapsed and condensed about 4.56 billion years ago.
Most of this matter compacted together to form the Sun, while the remainder formed planets, asteroids, and smaller bodies.
Terrestrial vs. Jovian Planets
The outer planets—Jupiter, Saturn, Uranus, and Neptune—condensed at cold temperatures and are made mostly of hydrogen and helium. In contrast, the terrestrial planets (Mercury, Venus, Earth, and Mars), formed closer to the Sun, contain large amounts of iron, silicates (silicon and oxygen), magnesium, and other heavier elements that condense at high temperatures.
About 4 billion years ago, conditions... Continue reading "Planetary Formation, Geologic Time, and Earth's Core Composition" »