Chapter 26: History of Life on Earth and Human Evolution
Instructor: Dr. Subhankar Mandal
Course: BIO 182, General Biology II
Term: Fall 2025
Key Concepts
The Fossil Record
History of Life on Earth
Human Evolution
Origin of Life
The Big Bang occurred 13.8 billion years ago (bya) and is believed to have initiated the universe.
Our solar system formed 4.6 billion years ago.
Life is thought to have emerged between 4.0 and 3.5 billion years ago on Earth.
Fossils from 3.5 billion years ago show resemblance to modern cyanobacteria, indicating early life forms.
The Fossil Record
Fossils are defined as the preserved remains of past life on Earth.
Paleontologists specialize in the study of fossils.
Many fossils are found in sedimentary rocks formed from particles of older rocks (sediments).
These sediments accumulate due to erosion and pressure create new rock layers.
When organisms are buried quickly, their hard parts can be replaced by minerals through processes like permineralization.
The depth of rock layers indicates their age; older rock layers tend to be found deeper within the Earth's crust.
History of Life on Earth
The geological time scale outlines the timeline of Earth's history from its formation (4.55 billion years ago) to the present.
This timeline is divided into four eons:
Hadean
Archaean
Proterozoic
Phanerozoic
The Precambrian period includes the Hadean, Archaean, and Proterozoic eons.
Each eon can be further divided into eras and periods.
Major Time Events
The geological time scale includes significant milestones in evolutionary history, as illustrated in Figure 26.4.
Notable events include:
7 million years ago: First hominoids appear
135 million years ago: Flowering plants first appear
Major milestones timeline:
1.5 billion years ago: Multicellular eukaryotic organisms first appear
1.8 billion years ago: Eukaryotic cells first appear
3.5 billion years ago: Fossils of primitive cyanobacteria found
Greek classification of organisms based on these timelines and species evolution observed in fossil records.
Changes in Species
Changes in living organisms can be attributed to:
Genetic changes within populations
Environmental changes affecting survival and reproduction
These changes can allow new types of organisms to flourish, but can also lead to mass extinctions, defined as the complete loss of a species or groups of species.
Major Environmental Changes
Factors contributing to species changes include:
Temperature fluctuations
Atmospheric composition (e.g., amounts of oxygen)
Landmass shifts
Floods and Glaciation events
Volcanic eruptions
Meteorite impacts
Mass Extinctions
There have been five large mass extinction events in Earth’s history associated with major geological transitions. These include:
Ordovician, Devonian, Permian, Triassic, and Cretaceous extinction events.
The boundaries between geological time periods are often marked by these extinction events.
Currently, we are witnessing a sixth mass extinction, attributed to rapid extinction of many species due to human activities.
Proterozoic Eon
Multicellular Eukaryotes
Multicellular eukaryotes emerged approximately 1.5 billion years ago.
Two theoretical origins of multicellularity include:
Individuals forming colonies
A single cell dividing and remaining attached to form a multicellular organism.
Volvocine green algae exhibit varying degrees of multicellularity, showcasing early evolutionary transitions.
Emergent Properties
The formation of different cell types is an emergent property of multicellularity, resulting from complex interactions between cells.
Example: Volvox aureus, consisting of 1,000 to 2,000 cells, demonstrates two cell types: somatic and reproductive cells.
First Animals
Multicellular invertebrates were the first animals to appear toward the end of the Proterozoic eon, many exhibiting bilateral symmetry that facilitates locomotion.
Phanerozoic Eon
Characterized by the extensive proliferation of multicellular eukaryotic life from 543 million years ago to the present.
Divided into three principal eras:
Paleozoic Era
Mesozoic Era
Cenozoic Era
Paleozoic Era (543 to 248 million years ago)
Comprised of multiple periods:
Cambrian, Ordovician, Silurian, Devonian, Carboniferous, and Permian periods.
Cambrian Period
Occurring from 543 to 490 million years ago, characterized by warm and wet climates with no ice at the poles.
Notable for the Cambrian Explosion, a rapid increase in diversity of animal species, possibly due to:
Evolution of shells allowing animals to exploit new environments
Increased atmospheric oxygen fostering animal diversity
An "evolutionary arms race" between species leading to diversification.
Ordovician Period
Lasted from 490 to 443 million years ago, featuring a diverse group of marine invertebrates (e.g., trilobites and brachiopods).
The first primitive land plants and arthropods invaded land.
An abrupt climate change towards the end of the period led to a mass extinction where over 60% of marine invertebrates became extinct.
Silurian Period
From 443 to 417 million years ago, characterized by a relatively stable climate.
Introduction of significant new vertebrates and the evolution of early vascular plants, allowing terrestrial colonization.
Devonian Period
Spanning 417 to 354 million years ago, marked by a major increase in terrestrial species and the emergence of insects and tetrapods (amphibians).
The Age of Fishes was defined by a great flourishing of fish species, with some prolonged extinctions occurring near the period’s end.
Carboniferous Period
Occurred 354 to 290 million years ago; rich coal deposits formed from extensive forested swamps.
Characterized by the diversification of plants and animals, and the emergence of flying insects and the first amniotic eggs in reptiles.
Permian Period
Extended from 290 to 248 million years ago.
Continental drift formed the supercontinent Pangaea, leading to drier interior regions and shifts to dominant gymnosperms.
At the end of this period, a mass extinction event occurred, resulting in the extinction of 90 to 95% of marine species due to possible glaciations or volcanic eruptions.
Mesozoic Era
Defined by the Permian extinction, denoting the transition into the Age of Dinosaurs (248 to 65 million years ago).
Characterized by consistently hot climates and dry terrestrial environments.
Divided into three periods:
Triassic, Jurassic, and Cretaceous periods.
Triassic Period
Spanning 248 to 206 million years ago, overrun by reptiles and the first dinosaurs.
First true mammals emerged alongside dominant gymnosperms.
Jurassic Period
Lasted 206 to 144 million years ago, where gymnosperms continued to dominate and some dinosaurs grew to enormous size.
Early bird-like creatures also appeared, along with the presence of mammals, though not prevalent.
Cretaceous Period
Extending from 144 to 65 million years ago, dinosaurs remained the dominant terrestrial species.
Emergence of earliest flowering plants (angiosperms) occurred.
This period ended with another significant mass extinction event, wherein dinosaurs went extinct likely due to meteor impacts or volcanic eruptions.
Cenozoic Era
Spans most recent 65 million years, divided into Tertiary and Quaternary periods.
Transitional climatic conditions shifted from tropical to a colder, drier climate, often referred to as The Age of Mammals.
This era observes an incredible diversification of birds, fish, insects, and flowering plants.
Tertiary Period
From 65 to 1.8 million years ago, mammals expanded rapidly, with angiosperms becoming the dominant terrestrial plants.
Hominoids (includes humans and relatives such as chimpanzees and gorillas) appeared about 7 million years ago.
Quaternary Period
Lasting 1.8 million years ago to present, marked by periodic ice ages and widespread extinctions among mammals.
Significant evolutionary changes occurred in hominids, leading to the emergence of Homo sapiens approximately 200,000 years ago.
Human Evolution
Inquiry questions related to human evolution include:
How closely related are humans to their nonhuman relatives?
What evolutionary events led to the rise of modern humans?
Level of genetic variation among present-day humans.
Are humans still undergoing evolution?
Primate Evolution
Primates evolved from a group of small, arboreal, insect-eating mammals approximately 85 million years ago.
Characterized by traits including:
Binocular vision
Nails on digits instead of claws
Grasping hands
Larger brains relative to body size
Complex social structures and parenting behaviors
Taxonomic Groups of Primates
Strepsirrhini:
Small species like bush babies and lemurs, predominantly nocturnal.
Recognized for their wet noses with no fur at the tip.
Haplorrhini:
Features dry noses and fully forward-facing eyes; includes tarsiers and larger-brained anthropoids.
Further divided into:
Monkeys
Hominoidea: Includes gibbons, orangutans, gorillas, chimpanzees, and humans.
Differentiation between Monkeys and Hominoids
Monkeys typically possess tails, while hominoids do not.
Hominoids exhibit more mobile shoulder joints, broader rib cages, and shorter spines.
Humans are close relatives of chimpanzees and gorillas but did not evolve directly from them; all hominoids share a common ancestor.
Comparison of Genomes
Comparative analysis shows that the genomes of humans and chimpanzees differ by only 1.23%.
This is substantially less than the differences between mouse and rat genomes.
Proteomic analysis reveals that roughly 29% of all proteins are identical, with variations mainly due to single amino acid substitutions.
Genetic variability largely arises from chromosomal inversions and duplications, with some differences influencing speech development.
Bipedalism in Hominins
The divergence leading to modern humans occurred around 7 million years ago in Africa, differentiating a lineage of humans from other primates.
Bipedalism is the key characteristic that differentiates hominins from other apes, and it is associated with significant anatomical changes such as:
Foramen magnum being situated more toward the front of the skull
Broader pelvis to support bipedal weight
Enlarged lower limbs.
Progression of Hominin Species
Australopithecus afarensis:
First fossil discovered in South Africa; female skeleton known as “Lucy” found in Ethiopia.
Smaller than modern humans, with a facial structure and brain size similar to chimpanzees.
Exhibits significant sexual dimorphism and was bipedal.
Paranthropus:
Larger-boned hominins found in the 1930s; identified as a separate genus.
Primarily vegetarian with large jaws for grinding roots; went extinct around 1.5 to 2 million years ago.
Homo habilis:
Fossils found in Olduvai Gorge, Tanzania, estimated to be 2 million years old.
Characterized by a larger brain than Australopithecus and associated with stone tools.
Homo ergaster:
Likely arose from Homo habilis around 2 million years ago.
Had human-like facial structure and skull; considered the first to leave Africa.
Homo erectus:
Large hominin closely resembling modern humans but with heavier bones and slightly smaller brain size.
Evidence of tool use and cooking; spread out of Africa after their emergence over a million years ago.
Went extinct around 100,000 years ago.
Homo heidelbergensis:
Similar in form to modern humans, showed tool use for hunting; gave rise to Neanderthals, Denisovans, and Homo sapiens.
Homo neanderthalensis (Neanderthals):
Discovered in the Neander Valley of Germany; stockier and shorter with a larger brain than Homo sapiens.
Artifacts indicate they might have used speech; went extinct 40,000 to 30,000 years ago.
Denisovans:
Discovered through genetic testing of remains found in Denisova Cave, Siberia; likely distinct from Neanderthals and modern humans.
Estimated to have existed around 400,000 years ago and possibly coexisted with Neanderthals and modern humans.
Homo sapiens:
Our species, identified as “wise man”; slight smaller brain capacity than Neanderthals.
Factors leading to their endurance include lower energy needs, increased longevity, and advanced social structures.
Out-of-Africa Model
Evidence indicates that Homo sapiens evolved from Homo heidelbergensis in Africa about 200,000 years ago.
Some migrated from Africa, leading to the replacement of other hominid species like Neanderthals.
An alternative hypothesis, the multiregional hypothesis, suggests parallel evolution of human groups from Homo ergaster across various global regions, though this is less accepted.
Interbreeding Among Hominids
DNA studies show that Homo sapiens interbred with related hominid species throughout Europe and Asia.
Modern humans of African descent generally carry little Neanderthal or Denisovan DNA, whereas those of European descent have 1 to 4% from Neanderthals, with 20% of the Neanderthal genome represented.
Southeast Asians may show approximately 4 to 6% Denisovan DNA.
Are Humans Still Evolving?
Human evolution via natural selection continues to manifest. Examples of current adaptations include:
Disease resistance (e.g., bubonic plague)
Lactose tolerance in populations that consume dairy
The prevalence of blue eyes across some European populations over the past 10,000 years.
Genetic Variation in Modern Humans
Although humans display striking physical differences globally, genetic variation is relatively low.
Humans exhibit lower genetic variance compared to most other mammal species.
99.9% of human genetic variation consists of single nucleotide polymorphisms (SNPs).
With a genome of 3 billion base pairs, differences between individuals are about 4.5 million SNPs, equating to only 0.15% variation.
Minimal additional genetic variance can also be observed amongst geographically separated human populations.