This unit is ≈16% of the Biology, across 8 lessons. Full syllabus
AP Biology · Lesson 8 of 8 · Unit 7
Origins of life on Earth
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Understanding how abiotic chemistry transitioned into self-replicating biological systems anchors Unit 7’s evolutionary timeline. On the AP Biology exam, Topic 7.12 is tested through experimental scenarios investigating abiotic synthesis, geological timelines, and the catalytic properties of RNA.
By the end you’ll be able to
Describe the geological evidence that supports models of the origin of life on Earth.
Use the dates for Earth’s formation, the end of hostile conditions and the earliest fossil evidence to describe a plausible range of dates for the origin of life.
Describe the RNA world hypothesis and its three assumptions: RNA replication assured genetic continuity, base pairing was necessary for replication, and genetically encoded proteins were not involved as catalysts.
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State a null hypothesis or predict the results of an experiment testing an origin-of-life model.
What the exam asks
In Section I (Multiple Choice), you will encounter stimulus sets describing laboratory simulations of early Earth or extraterrestrial chemical analyses. You may be asked to link geological evidence to the timeline of life’s emergence or identify which biochemical observation supports the RNA world hypothesis.
In Section II (Free Response), this topic frequently appears in Question 1, Question 2, or Question 3 (Scientific Investigation). Expect to state a testable null hypothesis (H0) for an abiogenesis experiment, identify experimental controls, or predict how modifying primitive reaction conditions affects monomer or polymer accumulation.
Core ideas
Geological evidence and the timeline of life
Geological and paleontological evidence brackets the window during which life first appeared on Earth. You must know three benchmark dates (in billions of years ago, bya) and what they signify:
Milestone
Approximate Date
Significance for the Origin of Life
Formation of Earth
4.6 bya
Earth accretes from solar dust; temperatures are molten and asteroid bombardment is intense.
End of hostile conditions
3.9 bya
The planet cools enough for liquid water to condense into oceans; heavy bombardment subsides, setting the earliest possible boundary for life.
Earliest fossil evidence
3.5 bya
Fossilized stromatolites (layered microbial mats formed by ancient prokaryotes) provide the latest boundary by which life definitely existed.
Together, these dates provide a plausible range for the origin of life between 3.9 bya and 3.5 bya.
Models of abiotic synthesis
Before cells existed, organic molecules had to form without enzymes:
Abiotic synthesis of small organic molecules: Primitive inorganic precursors (such as H2O, CH4, , and ) reacted using environmental energy sources (lightning, UV radiation, or hydrothermal vent heat) to form amino acids and nitrogenous bases. Crucially, the early atmosphere lacked free oxygen gas (), making it a non-oxidizing environment where organic bonds could form without immediately degrading.
Meteorite transport: Alternatively, organic monomers formed in space and arrived on early Earth via meteorites.
Abiotic polymerization: Monomers joined into polymers (polypeptides and RNA) when concentrated on hot sand, clay, or rock surfaces, which acted as inorganic catalysts for dehydration synthesis.
Protocells: Self-assembling lipid vesicles enclosed these polymers, creating an internal chemical environment distinct from the surrounding ocean.