Most scientists agree that Earth is billions of years old
The conditions of the early planet and its atmosphere were very different from those of today
The solar system was formed by a condensing nebula, a cloud of gas and dust in space, about 4.6 billion years ago
Over time, most of the material in the nebula pulled together because of gravity, forming the Sun and planets of our solar system
Earth was violent and very hot for its first 700 million years, known as the Hadean eon
During the Hadean eon, many asteroids, meteorites, and comets struck the planet, releasing enormous amounts of heat
The early atmosphere contained compounds such as ammonia, water vapor, methane, and carbon dioxide
Free oxygen was not abundant until about 2 billion years ago, after the first forms of life had begun to evolve
Impacts on Earth became less frequent towards the end of the Hadean eon, allowing the planet to cool down
Once liquid water was present, organic compounds could be formed from inorganic materials
Living matter is organic, including sugars and amino acids
The leap that resulted in life on Earth required conditions other than just the presence of water
Several hypotheses propose how life began on Earth
Scientists have proposed hypotheses about early organic molecules, the evolution of cell structures, and early genetic material since the 1950s
Two general hypotheses about the appearance of life supporting molecules on early Earth are the Miller-Urey experiment and the meteorite hypothesis
The Miller-Urey experiment demonstrated that organic compounds could be made by passing an electrical current through a mixture of gases
Analysis of a meteorite revealed that organic molecules can be found in space, suggesting they could have been present when Earth formed or arrived through impacts
There are hypotheses about the formation of the first cells, including the iron-sulfide bubbles hypothesis and the lipid membrane hypothesis
The iron-sulfide bubbles hypothesis proposes that biological molecules combined in compartments of chimney-like structures, acting as the first cell membranes
The lipid membrane hypothesis suggests that lipid molecules spontaneously formed membrane-enclosed spheres, which may have given rise to the first true cells
A hypothesis gaining support proposes that RNA, rather than DNA, was the genetic material that stored information in living things on early Earth
Ribozymes are RNA molecules that can catalyze specific chemical reactions, suggesting RNA's role in early genetic material
RNA can replicate itself without additional enzymes, unlike DNA which needs enzymes for replication
RNA can catalyze reactions and copy itself, while DNA requires enzymes for replication
Single-celled organisms existed 3.8 billion years ago
Microbes have changed the physical and chemical composition of Earth
Eukaryotic cells may have evolved through endosymbiosis
The evolution of sexual reproduction led to increased diversity
Early single-celled organisms changed Earth's surface by depositing minerals and changed the atmosphere by giving off oxygen as a byproduct of photosynthesis
Stromatolites are evidence of Earth's early life, made by cyanobacteria which were among the first organisms on early Earth
Endosymbiosis is a relationship in which one organism lives within the body of another, benefiting both
Mitochondria and chloroplasts found in eukaryotic cells descended from ancestors of infection-causing bacteria and cyanobacteria, respectively
Sexual reproduction increases genetic variation, masking harmful mutations and bringing beneficial mutations together
Sexual reproduction may have resulted in an increase in the rate of evolution by natural selection, allowing populations to adapt quickly to new conditions
Recombination is an important source of genetic variation, resulting in many different phenotypes through the process of producing gametes and during crossing over in meiosis
Humans appeared late in Earth's history
Humans share a common ancestor with other primates