
Geobiology Course
Geobiology sits at the intersection of life, Earth, and deep time — and this course gives you the scientific tools to explore all three. From microbial ecosystems to mass extinctions, you'll learn how life and the planet have shaped each other across billions of years. Whether your focus is paleontology, planetary science, or environmental research, this course builds the rigorous foundation you need.
What you will learn:
This course covers the full scope of geobiology, from biogeochemical cycles and microbial metabolism to biosignature detection and astrobiology. You will learn how to read the rock record for evidence of ancient life, reconstruct paleoenvironments using geochemical proxies, and analyze major biological transitions including the Great Oxidation Event and mass extinctions. The curriculum also addresses modern geobiological systems, analytical laboratory methods, and quantitative modeling techniques. By the end, you will be equipped to design original geobiological research and communicate findings to both scientific and public audiences.
How you study in practice Geobiology Course
How you practice Geobiology Course
For companies that want to train their team
With Dedika for Business, the course includes exercises and examples tailored to your own business and the way your company needs.
Course content
8 Chapters • 39 LessonsDuration between 4 and 360 hours (you decide)
Chapter 1HideHide detailsSee detailsFoundations of Geobiology
Foundations of Geobiology
Lesson 1 • Fundamental Biogeochemical Cycles
Carbon, nitrogen, sulfur, and phosphorus cycles are examined as geobiological drivers. Understanding these cycles is prerequisite for interpreting biosignatures and Earth history.
Lesson 2 • Deep Time and Geological Timescales
Introduces the geological timescale and methods for reading Earth's rock record. Students develop intuition for the vast temporal scales central to geobiology.
Lesson 3 • Defining Geobiology as a Discipline
Geobiology's scope, history, and relationship to adjacent sciences are mapped. This context anchors all later technical content within a unified scientific framework.
Lesson 4 • Earth Systems and Life Interactions
Covers feedbacks between the biosphere, lithosphere, hydrosphere, and atmosphere. Students understand how life both responds to and reshapes Earth's physical systems.
Chapter 2HideHide detailsSee detailsMicrobial Life and Earth Processes
Microbial Life and Earth Processes
Lesson 1 • Biomineralization by Microorganisms
Covers biologically induced and controlled mineral precipitation by microbes. These processes produce diagnostic textures preserved in the rock record.
Lesson 2 • Microbial Diversity and Metabolism
Surveys the metabolic strategies microbes use to harvest energy from inorganic and organic substrates. This diversity underpins microbial roles in geochemical cycling.
Lesson 3 • Microbial Weathering of Minerals
Microbial dissolution and transformation of silicate and sulfide minerals are examined. Students link microbial activity to soil formation and elemental release.
Lesson 4 • Microbial Mats and Biofilms
Structured microbial communities are analyzed as geochemically active units. Their spatial organization creates steep chemical gradients that drive mineral transformations.
Lesson 5 • Subsurface Microbial Ecosystems
Deep subsurface environments host chemolithotrophic communities independent of sunlight. These systems reveal the limits of life and inform models of early Earth and other planets.
Chapter 3HideHide detailsSee detailsOrigin and Early Evolution of Life
Origin and Early Evolution of Life
Lesson 1 • Earliest Evidence of Life on Earth
The oldest putative biosignatures from Archean rocks are critically evaluated. Students apply biosignature criteria from Chapter 3 to assess claims of early life.
Lesson 2 • Origin of Eukaryotes and Endosymbiosis
Endosymbiotic theory and the geobiological context of eukaryote emergence are examined. Students link cellular complexity to environmental and ecological transitions.
Lesson 3 • Great Oxidation Event and Its Consequences
The rise of atmospheric oxygen around 2.4 billion years ago transformed Earth's surface chemistry. Students analyze causes, timing, and biological and geological consequences.
Lesson 4 • Evolution of Photosynthesis
The development of anoxygenic and oxygenic photosynthesis is traced through the rock record. Students connect photosynthetic evolution to planetary-scale geochemical change.
Lesson 5 • Prebiotic Chemistry and Abiogenesis
Chemical pathways leading to organic molecules and proto-cellular structures are examined. Students assess how early Earth environments may have facilitated life's origin.
Chapter 4HideHide detailsSee detailsBiosignatures and the Fossil Record
Biosignatures and the Fossil Record
Lesson 1 • Molecular Fossils and Biomarkers
Lipid biomarkers preserved in sedimentary rocks record the presence of specific biological groups. Students learn extraction, analysis, and interpretation of these molecular archives.
Lesson 2 • Types of Biosignatures
Morphological, chemical, and isotopic biosignatures are classified and compared. Recognizing each type is essential for interpreting ancient life in the rock record.
Lesson 3 • Microfossils and Their Interpretation
Techniques for identifying and authenticating microfossils in cherts and carbonates are covered. Students apply criteria to distinguish genuine microfossils from pseudofossils.
Lesson 4 • Stable Isotope Geobiology
Carbon, sulfur, and nitrogen isotope systems are applied to reconstruct biological activity. Isotopic fractionation patterns serve as quantitative biosignatures in ancient rocks.
Lesson 5 • Stromatolites as Biological Archives
Stromatolite morphology, formation mechanisms, and geological distribution are analyzed. Students use stromatolites as proxies for ancient microbial ecosystems and environmental conditions.
Chapter 5HideHide detailsSee detailsGeochemical Proxies and Paleoenvironments
Geochemical Proxies and Paleoenvironments
Lesson 1 • Ocean Chemistry Through Time
Redox state, salinity, and trace metal concentrations of ancient oceans are reconstructed. These records reveal how ocean chemistry co-evolved with life and atmosphere.
Lesson 2 • Integrating Proxies into Paleoenvironmental Models
Multiple proxy datasets are combined to construct coherent paleoenvironmental reconstructions. Students practice synthesizing conflicting proxy signals into robust interpretations.
Lesson 3 • Atmospheric Proxies and Paleoatmosphere
Methods for reconstructing ancient atmospheric oxygen and carbon dioxide levels are covered. Students connect atmospheric reconstructions to biological and climatic events.
Lesson 4 • Principles of Proxy Reconstruction
The logic of using chemical and physical signals in rocks as environmental proxies is established. Students learn to assess proxy fidelity, diagenetic alteration, and uncertainty.
Lesson 5 • Sedimentary Facies and Depositional Environments
Sedimentary rock types and facies associations are linked to specific depositional settings. Students use facies analysis to place biological events in their environmental context.
Chapter 6HideHide detailsSee detailsMajor Biological Transitions and Mass Extinctions
Major Biological Transitions and Mass Extinctions
Lesson 1 • Patterns and Causes of Mass Extinctions
The five major mass extinctions are analyzed for their geobiological signatures and causes. Students identify common environmental stressors and biological vulnerabilities.
Lesson 2 • Recovery and Radiation After Extinction
Post-extinction recovery dynamics and evolutionary radiations are examined across multiple events. Students analyze how survivors reshape ecosystems and drive new geobiological cycles.
Lesson 3 • Cambrian Explosion and Animal Origins
The rapid diversification of animal body plans in the Cambrian is examined through fossil and geochemical evidence. Students evaluate environmental triggers and ecological drivers.
Lesson 4 • Neoproterozoic Snowball Earth Events
Global glaciation events and their biological consequences are analyzed using sedimentary and isotopic evidence. Students connect extreme climate perturbations to evolutionary transitions.
Lesson 5 • End-Permian Extinction: A Case Study
The largest mass extinction is dissected using geochemical, paleontological, and sedimentological data. Students apply multi-proxy analysis to reconstruct the extinction mechanism.
Chapter 7HideHide detailsSee detailsModern Geobiological Systems and Environments
Modern Geobiological Systems and Environments
Lesson 1 • Soil Geobiology and Critical Zone Science
The critical zone from bedrock to canopy is analyzed as an integrated geobiological system. Students examine how organisms drive weathering, nutrient cycling, and soil development.
Lesson 2 • Wetlands, Peatlands, and Carbon Storage
Organic carbon accumulation in wetland and peatland systems is examined as a geobiological process. Students link microbial decomposition rates to long-term carbon burial.
Lesson 3 • Hydrothermal Vent Ecosystems
Chemosynthetic communities at mid-ocean ridges are examined as models of early Earth ecosystems. Students analyze energy flow, mineral precipitation, and community structure.
Lesson 4 • Carbonate Systems and Reef Geobiology
Biological carbonate production in reefs and shallow marine settings is analyzed. Students connect organism-scale calcification to basin-scale carbonate accumulation.
Lesson 5 • Extreme Environments as Geobiological Analogs
Hypersaline lakes, acid mine drainage, and polar environments are studied as analogs for ancient and extraterrestrial settings. Students evaluate habitability limits and biosignature preservation.
Chapter 8HideHide detailsSee detailsAstrobiology and the Search for Life
Astrobiology and the Search for Life
Lesson 1 • Ocean Worlds and Icy Moon Habitability
Subsurface oceans on Europa, Enceladus, and similar bodies are evaluated as potential habitats. Students connect deep-sea geobiology to extraterrestrial ocean environments.
Lesson 2 • Mars as a Geobiological Target
Mars's geological and geochemical history is evaluated for past and present habitability. Students apply geobiological proxy methods to interpret Mars mission data.
Lesson 3 • Habitability: Concepts and Requirements
The physical and chemical requirements for life as we know it are defined and evaluated. Students apply habitability criteria to assess environments on Earth and other worlds.
Lesson 4 • Panspermia and Life's Cosmic Context
Hypotheses for interplanetary transfer of life are evaluated against geobiological and physical evidence. Students place Earth's biosphere within a broader cosmic perspective.
Lesson 5 • Biosignature Detection in Planetary Science
Remote and in-situ biosignature detection methods are evaluated for planetary missions. Students design detection frameworks using geobiological principles established throughout the course.
Your valid completion certificate
This course is for you:
Geology student: wants to understand how life has driven Earth's chemical evolution.
Astrobiology enthusiast: seeks rigorous grounding before pursuing planetary habitability research.
Environmental scientist: needs deeper knowledge of microbial roles in geochemical systems.
Paleontology researcher: aims to interpret fossil evidence within broader Earth system contexts.
Biology graduate student: ready to connect evolutionary history to large-scale geological processes.
Science educator: building expertise to teach Earth history with biological and chemical depth.
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