Photosynthesis

Overview

Photosynthesis is a set of processes that plants, algae, and some bacteria use to convert light energy into chemical energy stored within organic compounds. The most common type—oxygenic photosynthesis—consumes carbon dioxide and water to produce oxygen and sugars such as glucose, the primary source of energy in cells. Photosynthesis has produced almost all of Earth's atmospheric oxygen, helps regulate the planet's carbon cycle, and supplies the energy that underlies most food chains.

Within cellular subunits called chloroplasts, photosynthesis primarily occurs in two stages. In light-dependent reactions, light is absorbed by chlorophyll and other pigments while water is decomposed to produce energy-carrying molecules and release oxygen.

In the Calvin cycle, RuBisCO—the most abundant protein on Earth—attaches carbon dioxide to a molecule called RuBP to create two, three-carbon molecules. The energetic molecules from the previous stage are then consumed to produce the building blocks of sugars. RuBP is also regenerated to restart the cycle, which runs six times to yield one glucose molecule.

Although these processes are impaired by rising temperatures, drought, and microplastics, some plants have evolved adaptations to cope with challenging environments, including leaf structures that enhance RuBisCO efficiency. Meanwhile, research is ongoing to develop artificial photosynthesis systems and improve photosynthesis for greater crop yields.

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