In 1952, scientist Stanley Miller and his mentor Harold Urey conducted a groundbreaking experiment, which is still widely regarded as the most important chemical experiment to explore the origin of life. This experiment not only simulated the environmental conditions of the early Earth, but also demonstrated for the first time how organic compounds can be synthesized from inorganic substances, further exploring how life may have originated from these basic chemicals. This experiment provided an important theoretical basis for the origin of life and triggered in-depth exploration of the early Earth environment and its chemical reactions.
Miller and Urey's experiments show how the environment on early Earth could have enabled the synthesis of organic molecules, a process that centered on a specific combination of ammonia, methane and hydrogen, and chemical reactions that followed the introduction of energy.
The main purpose of the Miller-Urey experiment was to simulate the chemical environment of the early Earth's atmosphere. Scientists chose three gases: methane (CH4), ammonia (NH3) and hydrogen (H2), mixed them in a ratio of 2:2:1, and added water (H2O). Then, using arc discharge to simulate the effects of lightning, the experimental team observed the formation process of organic molecules, especially the generation of amino acids.
Miller sealed the gases in a 5-liter glass bottle and connected it to a 500-milliliter bottle filled with water, a design that simulated the ocean and atmospheric conditions of early Earth. When water is heated to produce water vapor and mixed with gas, the arc discharge is initiated, forming a series of chemical reactions, and ultimately producing a variety of amino acids including glycine and alanine. There is no doubt that these findings provide important evidence for understanding the chemical basis of life.
During the first week of the experiment, the liquid collected from the bottom turned a deep red color, a phenomenon Miller interpreted as adsorption of organic matter, allowing these molecules to accumulate in the water.
The design of this experiment was inspired by several theories of the origin of life in the early 20th century, including the "primordial soup" theory of Russian scientist Alexander Oparin and British scientist J.B.S. Haldane. These theories hold that in the early oceans of the Earth, organic molecules must have been formed in a chemical reaction process due to the influence of light and heat, eventually leading to the emergence of life.
Miller's experiment successfully established a pathway for the transition from simple inorganic compounds to complex organic substances, which later led to many studies and experiments in this field.
Although Miller's experiments were imperfect at the time, scientists gradually realized that the basic conditions required for these synthesis processes might exist in high-energy environments, such as Earth after a massive impact.
Over time, the impact of the Miller-Urey experiment has been profound. Many modern experiments and studies build on its theoretical framework to further explore possible origins of life, including experiments simulating extraterrestrial environments or different atmospheric compositions.
For example, experiments in recent years have confirmed that even under different chemical combinations, such as changing the proportion of ammonia, the synthesis of amino acids can still be observed, which suggests that the environment of the early Earth may have been more diverse.
The Miller-Urey experiment not only provided the scientific community with a preliminary explanation for the origin of life, but also became a symbol that the transition from chemistry to life is possible. As technology develops, scientists are able to probe these reactions more deeply and explore the fundamental chemistry of life.
Recent studies of the early Earth's atmosphere have shown that the composition of the gases may be somewhat different from what was used in Miller's experiment, but what remains unchanged is that the significance and gravity of these chemical processes are still strong.
As we continue to discover new planets and moons in the universe, it makes us wonder: if the origin of life is not just a story on Earth, is it possible that life on other planets arose in a similar way?