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Origin of the Earth and of Life
Learning Objectives
After reading this chapter, students should be able to:
• Realize that the solar nebula formed from a cloud of interstellar gas
• Know that the Earth and the other terrestrial planets are 4.55 billion years old
• Know that the evidence for this age comes from radiometric dating of meteorites
• Understand how location in the solar nebula determined whether a planet became a
gas giant or a terrestrial planet.
• Understand that the moon was formed by a giant impact between the Earth and a
Mars-sized planetesimal
• Know how the early atmosphere and ocean formed from volatiles released from
impacts of comets and asteroids
• Realize that the Earth’s early atmosphere was drastically different from the present-
day atmosphere, with extremely low O2 and O3 levels and high CO2 levels.
• Know there are a number of theories on how life first arose, including a theory of
chemical evolution that results in an RNA-world.
• Know how the Urey-Miller experiment created amino acids, and what the
implications of this experiment were for the chemical evolution theory
• Realize that the gas mixture used in the Urey-Miller experiment probably does not
represent the atmosphere of the Earth when life first evolved
• Know what the RNA-world is and realize that many biologists support such a world
as a stepping stone towards the development of life because of RNA’s ability to self
replicate and encode protein production
• Consider the possibilities for prebiotic synthesis of glucose, and the RNA bases
• Consider theories for the evolution of life that involve prebiotic chemistry at
hydrothermal vents and in space
• Know that that most scientists agree that life had arisen by at least 3.5 billion years
ago, and that some believe life arose as early as 4.0 billion years ago
• Know what the Universal Tree of Life is, and its implications for the origin of life
• Offer multiple hypotheses explaining why methanogens are thought to be amongst
the earliest forms of life on Earth
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