Stanley Miller and Harold Urey performed the Miller-Urey experiment in 1953, which was a landmark experiment showing the possible origin of life on Earth under prebiotic conditions. In Miller's experiment, a mixture of gases like methane, ammonia, hydrogen, and water vapour thought to be representative of the early Earth's atmosphere was exposed to electrical sparks simulating lightning. The Stanley Miller-Urey experiment is a bedrock experiment for understanding the chemical origins of life. This is part of the chapter Evolution in Biology.
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The Miller-Urey experiment was one of the key studies that Stanley Miller and Harold Urey conducted in 1953. It simulated the early Earth environment to test abiogenesis associated with the spontaneous eruption of simple life forms from non-living matter.
The importance of this experiment lies in the fact that it offers a basis where simple organic compounds, could be built up from inorganic precursors under conditions that might have existed on primordial Earth.
Previous to the Miller-Urey experiment, several leading theories on evolution were mostly speculative. The works by Alexander Oparin and J.B.S. Haldane speculated that early Earth atmospheres could have been such that the spontaneous generation of organic compounds from simple molecules could occur. This was not tested until Miller and Urey came up with their so-called experiment.
The scientific environment of the early 1950s was ripe for a question about life's origin. Advances in chemistry and biological research set the stage for Miller and Urey to test the abiogenesis theory by simulating a controlled laboratory experiment.
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The main purpose of the Miller-Urey experiment was to find the conditions of primitive Earth. This later proved to be an experiment conducted to explain whether such conditions gave rise to organic compounds necessary for life.
Glass Tubes and Flasks: These were used to contain the experimental mixture and provide the medium through which gases could circulate.
Electrodes: These supplied electrical sparks that simulated lightning.
Gas Mixture Introduction
A gas mixture of Methane gas, CH₄, with Ammonia NH₃, Hydrogen, H₂, and Water Vapour, H₂O was introduced into a closed system of glass tubes and flasks.
Electrical Stimulation
Electrical sparks were created with electrodes, mimicking lightning storms that are believed to have been common on primitive Earth.
Cooling and Condensation
The mixture is allowed to cool, and the gases condensed back into the liquid water trap.
Collection and Analysis
After a week, the liquid collected was analysed, and the presence of organic compounds was detected.
The experiment produced a wide array of organic compounds including amino acids, which are, of course, the very building blocks of proteins and thus some of the prime constituents of living cells. This was an important discovery in terms of actually providing empirical evidence that life from simple inorganic molecules could have evolved under the right conditions.
Organic Compound Detected
Compound | Concentration (µM) |
Glycine | 50 |
Alanine | 20 |
Aspartic Acid | 15 |
Glutamic Acid | 10 |
One of the major criticisms against the Miller-Urey experiment lies in the composition of the atmosphere that was used. Miller and Urey held that the primitive atmosphere was very strongly reducing, rich in CH₄, NH₃, H₂, and H₂O. However, subsequent experiments suggested that early Earth's atmosphere might have been much less reducing and probably made of carbon dioxide, nitrogen, and water vapour, with a trace of hydrogen. This might then affect radically the kinds of organic molecules produced as a result of the different atmospheric compositions.
Electrical sparks imitated lightning as the energy source in the experiment, which would correspond to one plausible energy source for prebiotic chemistry. Other possible sources of energy include ultraviolet radiation, volcanic activity, and hydrothermal vents. Such alternative energy sources have been tested in other experiments, with equivocal results, suggesting that pathways for the origin of life can be much more diverse than that indicated by this classic experiment.
Given its pristine, controlled conditions, this experiment in the laboratory does not account for the impurities, catalytic surfaces, and variety of minerals found on early Earth. Under realistic conditions, several variables would have existed that could have affected the actual synthesis and stability of the organic molecules.
Alexander Oparin and J.B.S. Haldane postulated that life on early Earth began through a gradual chemical evolution of carbon-based molecules in a "primordial soup." While growing organic molecules in the lab under prebiotic conditions, the Miller-Urey experiment provided evidence for this hypothesis however, it essentially only tested a very small part of what Oparin and Haldane had in mind. Their theories generally envisioned a longer time frame and a much broader set of chemical processes.
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The Miller-Urey experiment provided a simulation of what was considered to be early Earth conditions and tried to show that, in fact, under these conditions, the organic compounds necessary for life can be formed.
The gases used in the Miller-Urey experiment consisted of methane CH₄, ammonia NH₃, hydrogen H₂, and, of course, water vapour H₂O.
Several organic compounds were produced in this experiment. At the top of the list, it produced amino acids like glycine, alanine, aspartic, and glutamic acid. These proved that simple organic molecules could be built up from inorganic precursors under conditions thought to have prevailed on early Earth.
The Miller-Urey experiment remains important because it furnished the first experimental support for in vitro abiogenesis—showing that some of the organic compounds essential for life could form under prebiotic conditions. It is one of the seminal discoveries in the history of the advancement of theories on the origin of life.
Some of the objections to the Miller-Urey experiment relate to the realism of the atmospheric mixture used in the experiment. Recent analyses of early Earth's atmosphere suggested it might have been far less reducing than earlier assumed.
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