Jove
Visualize
Contact Us
JoVE
x logofacebook logolinkedin logoyoutube logo
ABOUT JoVE
OverviewLeadershipBlogJoVE Help Center
AUTHORS
Publishing ProcessEditorial BoardScope & PoliciesPeer ReviewFAQSubmit
LIBRARIANS
TestimonialsSubscriptionsAccessResourcesLibrary Advisory BoardFAQ
RESEARCH
JoVE JournalMethods CollectionsJoVE Encyclopedia of ExperimentsArchive
EDUCATION
JoVE CoreJoVE BusinessJoVE Science EducationJoVE Lab ManualFaculty Resource CenterFaculty Site
Terms & Conditions of Use
Privacy Policy
Policies

Related Concept Videos

What is Weather?01:07

What is Weather?

Overview
Global Climate Change01:50

Global Climate Change

Throughout its ~4.5 billion year history, the Earth has experienced periods of warming and cooling. However, the current drastic increase in global temperatures is well outside of the Earth’s cyclic norms, and evidence for human-caused global climate change is compelling. Paleoclimatology, the study of ancient climate conditions, provides ample evidence for human-caused global climate change by comparing recent conditions with those in the past.
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
What is Evolutionary History?02:35

What is Evolutionary History?

Scientists record evolutionary history by analyzing fossil, morphological, and genetic data. The fossil record documents the history of life on Earth and provides evidence for evolution. However, both fossil and living organisms offer evidence that outlines Earth’s evolutionary history.Phylogenetic trees illustrate the evolutionary relationships among these organisms. Scientists infer organisms’ common ancestry by evaluating shared morphological and genetic characteristics. Together, the fossil...
Conditions on Early Earth02:06

Conditions on Early Earth

Around 4 billion years ago, oceans began to condense on earth while volcanic eruptions released nitrogen, carbon dioxide, methane, ammonia, and hydrogen into the primordial atmosphere. However, organisms with the characteristics of life were not initially present on earth. Scientists have used experimentation to determine how organisms evolved that could grow, reproduce, and maintain an internal environment.
Origin of Photosynthesis01:26

Origin of Photosynthesis

Photosynthesis represents a fundamental biological process that transformed Earth's atmosphere and paved the way for complex life. Emerging roughly 3.4–3.8 billion years ago, the earliest photosynthetic organisms harnessed light energy to produce organic compounds. These anoxygenic phototrophs used electron donors like hydrogen sulfide (H₂S) or ferrous iron (Fe²⁺), rather than water, and did not release molecular oxygen (O₂) as a byproduct. Various groups, including green sulfur and purple...

You might also read

Related Articles

Articles linked to this work by shared authors, journal, and citation graph.

Sort by
Same author

Comparison between ozone column depths and methane lifetimes computed by one- and three-dimensional models at different atmospheric O<sub>2</sub> levels.

Royal Society open science·2023
Same author

Greenhouse warming by nitrous oxide and methane in the Proterozoic Eon.

Geobiology·2011
Same author

Low pCO2 in the pore water, not in the Archean air.

Nature·2011
Same author

Mass-independent fractionation of sulfur isotopes in Archean sediments: strong evidence for an anoxic Archean atmosphere.

Astrobiology·2002
Same author

Irradiated interplanetary dust particles as a possible solution for the deuterium/hydrogen paradox of Earth's oceans.

Journal of geophysical research·2001
Same author

Synthetic spectra of simulated terrestrial atmospheres containing possible biomarker gases.

Icarus·2001
Same journal

A native sulfur deposit in Gale crater, Mars.

Science (New York, N.Y.)·2026
Same journal

Coordinated demise of harmful algal blooms.

Science (New York, N.Y.)·2026
Same journal

Genetic effects put into context.

Science (New York, N.Y.)·2026
Same journal

Bacteria share proteins to survive antibiotics.

Science (New York, N.Y.)·2026
Same journal

Impacts shaped Earth's first continents.

Science (New York, N.Y.)·2026
Same journal

Erratum for the Report "Covalently bonded single-molecule junctions with stable and reversible photoswitched conductivity" by C. Jia <i>et al</i>.

Science (New York, N.Y.)·2026
See all related articles

Related Experiment Video

Updated: Jun 29, 2026

Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface
13:27

Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface

Published on: June 8, 2015

Earth's early atmosphere.

J F Kasting1

  • 1Department of Geosciences, The Pennsylvania State University, University Park 16802.

Science (New York, N.Y.)
|February 12, 1993
PubMed
Summary
This summary is machine-generated.

Early Earth

Keywords:
NASA Discipline ExobiologyNASA Discipline Number 52-30NASA Program ExobiologyNon-NASA Center

More Related Videos

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
06:29

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment

Published on: February 27, 2021

Using Generative Art to Convey Past and Future Climate Transitions
06:10

Using Generative Art to Convey Past and Future Climate Transitions

Published on: March 31, 2023

Related Experiment Videos

Last Updated: Jun 29, 2026

Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface
13:27

Exploring the Effects of Atmospheric Forcings on Evaporation: Experimental Integration of the Atmospheric Boundary Layer and Shallow Subsurface

Published on: June 8, 2015

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment
06:29

Simulation of Early Earth Hydrothermal Chimneys in a Thermal Gradient Environment

Published on: February 27, 2021

Using Generative Art to Convey Past and Future Climate Transitions
06:10

Using Generative Art to Convey Past and Future Climate Transitions

Published on: March 31, 2023

Area of Science:

  • Geosciences
  • Paleoclimatology
  • Astrobiology

Background:

  • Atmospheric composition and climate evolution on early Earth are not fully understood.
  • Key uncertainties exist regarding the timing and drivers of atmospheric oxygenation.
  • The magnitude of the early greenhouse effect needed to counteract lower solar luminosity remains speculative.

Purpose of the Study:

  • To investigate the evolution of Earth's early atmosphere and climate.
  • To address uncertainties in the timing and causes of atmospheric oxygenation.
  • To refine estimates of early atmospheric greenhouse gas concentrations.

Main Methods:

  • This study synthesizes existing research and theoretical models on early Earth atmospheric evolution.
  • It analyzes geological evidence for oxygenation events and greenhouse gas levels.
  • Comparative planetology approaches may be considered.

Main Results:

  • While general trends of increasing oxygen and a stronger early greenhouse effect are accepted, precise details remain elusive.
  • The rise of oxygen around 2.0 billion years ago is a significant event, but its triggers are debated.
  • Required levels of carbon dioxide and other greenhouse gases for early climate regulation are still under investigation.

Conclusions:

  • Resolving uncertainties in early atmospheric composition is crucial for understanding life's evolution on Earth.
  • Accurate reconstructions of past atmospheres aid in the search for extraterrestrial life on exoplanets.
  • Further research is needed to fully elucidate the complex processes governing early planetary atmospheres.