Biology 2 · Study notes
Origin and History of Life
On this page 4 sections
The college version
Main notes
Life on Earth began roughly 3.5 to 3.8 billion years ago, less than a billion years after the planet formed about 4.6 billion years ago. This chapter traces how life arose from non-living chemistry, how the deep history of the planet is divided into eons and eras, and how catastrophe and innovation repeatedly reshaped the biosphere. Every organism alive today, from bacteria to humans, descends from that same origin and carries its traces in cells, ribosomes, and genes. The story sets the stage for the diversity and phylogeny chapters that follow, which organize the living descendants of that origin into a single family tree.
Abiogenesis Hypotheses
For centuries many naturalists accepted spontaneous generation, the idea that complex organisms arise directly from non-living matter, such as maggots appearing in rotting meat. In 1668 Francesco Redi showed that flies, not meat, produce maggots, and in 1861 Louis Pasteur's swan-neck flask experiments disproved spontaneous generation for all observable cases. Pasteur's work established biogenesis, the principle that life arises only from existing life, yet it also raised the deepest question of biology: if life cannot arise from non-life today, how did it arise at all? The answer is abiogenesis, the origin of life from simple non-living chemistry under conditions very different from the present.
In the 1920s Alexander Oparin and J. B. S. Haldane independently proposed that the early atmosphere was reducing, rich in methane, ammonia, and hydrogen, with almost no free oxygen. Lightning and ultraviolet light could drive those gases to form organic monomers, which would accumulate in the oceans as a primordial soup and later assemble into larger molecules. In 1953 Stanley Miller and Harold Urey tested the idea in the laboratory. They sparked a sealed mixture of water, methane, ammonia, and hydrogen and recovered several amino acids and other organic compounds within days, showing that the building blocks of life can form from simple chemistry alone.
Later models add other energy sources and settings. Hydrothermal vents on the deep seafloor release minerals and maintain chemical gradients that can power the formation of organic molecules, so some hypotheses place the origin of life there rather than in a sunlit surface ocean. Meteorites and comets delivered organic compounds, including amino acids, that formed in space, so the early Earth also received imported building blocks. Whatever the venue, the general pathway runs from monomers through polymers to cell-like droplets called protobionts, spheres of lipids that grow, split, and concentrate molecules but cannot yet replicate. The endpoint of this process is the last universal common ancestor, or LUCA, the population from which all living things descend.
The proposed sequence from chemistry to cells is an ordered chain:
1. Small monomers such as amino acids and nucleotides form from simple gases.
2. Monomers join into polymers such as proteins and nucleic acids.
3. Lipids self-assemble into protobionts that enclose and concentrate molecules.
4. A self-replicating polymer emerges inside a protobiont.
5. Selection favors replicators that copy more accurately and survive better.
6. LUCA gives rise to all living cells.Common Mistake: Assuming Pasteur disproved abiogenesis. Pasteur only showed that life does not arise from non-life under modern conditions. The origin of life happened on early Earth, under a different atmosphere, over hundreds of millions of years.
ELI-10
Think of a big pot of warm soup left on a stove for a very long time. The ingredients drift and bump into each other, and occasionally they stick together into something new. Scientists think the early ocean worked like that pot. Simple pieces gradually joined into bigger ones until something could copy itself and count as alive.
The RNA World
A replicator made of protein could not copy itself, and a replicator made of DNA would need protein helpers to read it. The RNA world hypothesis resolves this chicken-and-egg problem: early life may have run on RNA, a molecule that can both store information and catalyze reactions. Catalytic RNA molecules are called ribozymes, discovered in the 1980s by Thomas Cech and Sidney Altman, who shared the 1990 Nobel Prize in Chemistry for the work. Their existence proved that a single molecule can carry hereditary information and speed up chemistry, exactly what the first replicator needed.
RNA solves the origin problem, but it is fragile and copies poorly. Natural selection then drove a division of labor. DNA became the stable archive of genetic information, and proteins, built from RNA templates, took over nearly all catalytic work because they can fold into far more shapes. The modern cell still preserves molecular fossils of the RNA world. Ribosomes, the machines that build proteins in every cell, use RNA as their catalytic core, and the energy currency ATP is made by an enzyme whose active core is RNA.
Common Mistake: Thinking the RNA world was a world of RNA cells. It was a stage of free molecules and protobionts, not cells, and RNA did not vanish when it was replaced. It survives inside every modern cell.
ELI-10
Picture one tool that is both a recipe book and a chef. The book tells you what to cook, and it also does the cooking itself. That single tool is like RNA, which holds instructions and speeds up chemical reactions at the same time. Later, cells split the job. A sturdy storage box called DNA kept the recipes, and fast chefs called proteins did the cooking.
The Geologic Timeline
Geologists divide Earth's history into eons, eras, and periods, with boundaries marked by major changes in the rock record. The Hadean eon (4.6 to 4.0 billion years ago) was the age of planet formation, when the young Earth was molten and repeatedly struck by large bodies. The Archean eon (4.0 to 2.5 billion years ago) saw the first life, the rise of prokaryotes, and the first photosynthetic cyanobacteria, whose layered mats built the oldest fossils, stromatolites, dating to about 3.5 billion years ago. By about 2.4 billion years ago, oxygen released by cyanobacteria triggered the Great Oxidation Event, which poisoned many anaerobic organisms while making oxygen-based metabolism possible.
The Proterozoic eon (2.5 billion to 541 million years ago) brought the first eukaryotes about 2 billion years ago, multicellular organisms by roughly 1 billion years ago, and the first simple animals near its end. The Phanerozoic eon, which began 541 million years ago, contains nearly all familiar life and is divided into three eras. The Paleozoic era (541 to 252 million years ago) opened with the Cambrian explosion, a rapid appearance of nearly all major animal body plans, followed by the colonization of land by plants about 470 million years ago and later by arthropods and vertebrates. The Mesozoic era (252 to 66 million years ago) was the age of reptiles and dinosaurs, with mammals present but small. The Cenozoic era (66 million years ago to today) began after the loss of the non-avian dinosaurs and saw the radiation of mammals and birds and the appearance of the human lineage only about 300,000 years ago.
| Eon | Dates | Key events |
|---|---|---|
| Hadean | 4.6 to 4.0 billion years ago | Planet formation, molten surface, heavy bombardment |
| Archean | 4.0 to 2.5 billion years ago | First life, prokaryotes, stromatolites, Great Oxidation Event |
| Proterozoic | 2.5 billion to 541 million years ago | Eukaryotes, endosymbiosis, multicellularity, first animals |
| Phanerozoic | 541 million years ago to present | Cambrian explosion, land colonization, dinosaurs, mammals, humans |
ELI-10
If Earth's whole history were squeezed into one year, the first cells would appear around March. Animals with hard shells would show up only in late November. The dinosaurs would rule for about a week in December and then vanish. Humans would arrive in the final minutes of New Year's Eve. Most of the calendar passes before anything big is alive.
The Big Five Mass Extinctions
The fossil record occasionally shows sudden, widespread loss of species, events called mass extinctions. The most severe are the big five. The end-Ordovician extinction about 444 million years ago followed rapid glaciation and eliminated roughly 85 percent of marine species. The Late Devonian extinction about 372 million years ago struck reefs and marine life, possibly through ocean anoxia. The end-Permian extinction about 252 million years ago was the largest of all, killing about 96 percent of marine species and roughly 70 percent of terrestrial vertebrate families, likely driven by the Siberian Traps volcanic eruptions and their runaway climate consequences. The end-Triassic extinction about 201 million years ago cleared space for the dinosaurs, and the end-Cretaceous extinction about 66 million years ago, caused by the Chicxulub asteroid impact, ended the non-avian dinosaurs while sparing mammals, birds, and other lineages.
Extinctions are not only destructive. They remove dominant competitors and open ecological space, allowing survivors to radiate in adaptive radiations. After 66 million years ago, mammals diversified into the roles left empty by the dinosaurs, producing everything from whales to bats to primates, and birds expanded in parallel. Many biologists argue that human activity is now driving a sixth mass extinction at a pace far faster than most of the big five.
| Extinction | Time | Likely cause |
|---|---|---|
| End-Ordovician | about 444 million years ago | Rapid glaciation and sea-level change |
| Late Devonian | about 372 million years ago | Ocean anoxia, possibly linked to plant spread |
| End-Permian | about 252 million years ago | Siberian Traps volcanism, runaway greenhouse |
| End-Triassic | about 201 million years ago | Volcanism during the breakup of Pangaea |
| End-Cretaceous | about 66 million years ago | Chicxulub asteroid impact |
ELI-10
Imagine a card game where most of the cards are suddenly swept off the table. The few cards left behind have the whole table to themselves. New cards multiply and fill the space, and the game looks completely different afterward. That is how mass extinctions work in nature.
Major Evolutionary Transitions
Major transitions are steps in which life reorganized into new units: molecules into cells, simple cells into complex cells, single cells into multicellular organisms, and individuals into societies. The transition to the eukaryotic cell depended on endosymbiosis, a process championed by Lynn Margulis in the 1960s. In the endosymbiotic theory, an early eukaryote engulfed an aerobic bacterium that became the mitochondrion, and later engulfed a cyanobacterium that became the chloroplast. The evidence is powerful: both organelles have their own circular DNA, divide independently, and are about the size of bacteria, and modern cells cannot function without their ancient partners.
The sequence of events is well supported:
1. An early eukaryote engulfs a small aerobic bacterium without digesting it.
2. The bacterium supplies extra energy in exchange for shelter and nutrients.
3. The partnership becomes permanent and the bacterium becomes the mitochondrion.
4. Later, a cyanobacterium is engulfed and becomes the chloroplast.
5. The organelles are passed to all descendants through the egg cell.Common Mistake: Confusing the two engulfed bacteria. The mitochondrion descends from an aerobic bacterium, while the chloroplast descends from a cyanobacterium. They entered the eukaryotic cell at different times and gave rise to different organelles.
The transition to multicellularity happened independently many times, in algae, fungi, plants, and animals. A single-celled ancestor forms a colony, cells specialize, and eventually no cell can survive alone, so the group becomes the unit of selection. This allowed bodies of enormous size and complexity and required new systems of cell-to-cell communication. The colonization of land was another transition with huge consequences. Plants evolved from green algae and reached land about 470 million years ago, transforming soils and the atmosphere; arthropods followed, and later vertebrates arrived through lobe-finned fish like Tiktaalik (about 375 million years ago), which gave rise to the tetrapods.
The final transition, unique among known life, was the evolution of humans. The lineage leading to modern humans split from chimpanzees about 6 to 7 million years ago, and Homo sapiens appeared roughly 300,000 years ago. With large brains, culture, and technology, humans became the first species able to alter the entire biosphere, which is why this deep history still matters today.
ELI-10
A single worker can only do small jobs. Join thousands of workers and they can build a city where each person has a specialty. Cells made the same change when they teamed up into large bodies. Different cells took different jobs, and the whole body worked as one team.
High-Yield:
- Earth formed about 4.6 billion years ago and the first life appeared 3.5 to 3.8 billion years ago.
- The end-Permian extinction was the largest, killing about 96 percent of marine species, not the end-Cretaceous.
- The end-Cretaceous extinction about 66 million years ago is the one that ended the non-avian dinosaurs.
- Eons in order are Hadean, Archean, Proterozoic, Phanerozoic, and the Phanerozoic eras are Paleozoic, Mesozoic, Cenozoic.
- Mitochondria and chloroplasts are living evidence that eukaryotes arose by endosymbiosis.
Quick Review
- Earth formed about 4.6 billion years ago, and the first life appeared roughly 3.5 to 3.8 billion years ago.
- Miller and Urey showed in 1953 that amino acids form from simple gases under simulated early conditions.
- The RNA world hypothesis proposes that catalytic RNA was the first replicator, and ribozymes still survive in ribosomes today.
- Geologic time is organized into eons, with the Phanerozoic containing the Paleozoic, Mesozoic, and Cenozoic eras.
- The Cambrian explosion about 541 million years ago produced nearly all major animal body plans.
- The big five mass extinctions include the end-Permian about 252 million years ago, the largest, and the end-Cretaceous about 66 million years ago, which killed the non-avian dinosaurs.
- Eukaryotes arose through endosymbiosis, when engulfed bacteria became mitochondria and chloroplasts.
- Humans appeared about 300,000 years ago, the latest of several major evolutionary transitions.
Key terms
Key terms are emphasized and defined within the main notes.
Important formulas or processes
See the formulas, procedures, and process blocks in the main notes where applicable.
Common mistakes
See the labeled common-mistake callouts in the main notes where present.
Key takeaway
Use the quick-review or recap section in the main notes.
Quick check
5 questions here, of 12 in this lesson’s practice set. Answers stay hidden until you check.
Some researchers once argued that life could not arise from nonliving matter and must have been carried to Earth from elsewhere in space. Which evidence best supports abiogenesis, the origin of life from nonliving chemicals, instead?
In the Miller-Urey experiment, a sealed flask of gases representing the early atmosphere was zapped with electric sparks meant to stand in for lightning, and the products were collected. What did the experiment demonstrate?
According to the RNA world hypothesis, RNA, not DNA or protein, was the first molecule of heredity and catalysis. Which property makes RNA the best candidate for this early role?
In the laboratory, molecules can assemble into protobionts, droplet-like structures with a membrane. Why do scientists consider protobionts important for understanding the origin of cells?
Study tools & related lessonsYou’ll learn to · Related
You’ll learn to
- Review and explain the concepts presented in this lesson.
Educational content only. It is not medical, legal or professional advice. Found an error? Tell us.

