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Origin of Photosynthesis01:26

Origin of Photosynthesis

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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...
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The Calvin Cycle01:40

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OverviewOxygenic photosynthesis plays a central role in the global carbon and oxygen cycles. The carbohydrates produced support nearly all food webs, while the oxygen by‑product enables aerobic life.Light‑dependent and light‑independent reactionsPhotosynthesis occurs in two main stages, each in a different part of the chloroplast: light‑dependent reactions and light‑independent reactions, also called the Calvin‑Benson cycle or simply the Calvin...
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The Anatomy of Chloroplasts01:08

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Green algae and plants, including green stems and unripe fruit, harbor specialized organelles called chloroplasts to carry out photosynthesis. They coordinate both stages of photosynthesis — the light-dependent reactions and the light-independent reactions. The light-dependent reactions use sunlight to release oxygen and produce chemical energy in the form of ATP and NADPH, and the light-independent reactions capture CO2 and use ATP and NADPH to produce sugar.
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Origin of Cellular Life01:24

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The origin of life on Earth is a complex and enigmatic event rooted in ancient biochemical processes and geological conditions. Experimental evidence supports the hypothesis that life began with the spontaneous formation of organic molecules such as RNA nucleotides, amino acids, and lipids under early Earth conditions. Factors like volcanic activity, intense UV radiation, and a reducing atmosphere without free oxygen likely facilitated these reactions. Hydrothermal vents on the ocean floor are...
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Oxygenic Photosynthesis01:26

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Oxygenic photosynthesis is a fundamental process in which light energy is harnessed to drive the oxidation of water, leading to the production of molecular oxygen (O₂), adenosine triphosphate (ATP), and nicotinamide adenine dinucleotide phosphate (NADPH). This process is essential for sustaining aerobic life on Earth and is primarily carried out by cyanobacteria, algae, and plants. The core of oxygenic photosynthesis lies in the thylakoid membranes, where chlorophyll pigments facilitate...
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What is Photosynthesis?00:39

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Photosynthesis is a multipart, biochemical process that occurs in plants as well as in some bacteria. It captures carbon dioxide and solar energy to produce glucose. Glucose stores chemical energy in the form of carbohydrates. The overall biochemical formula of photosynthesis is 6 CO2 + 6 H2O + Light energy → C6H12O6 + 6 O2. Photosynthesis releases oxygen into the atmosphere and is largely responsible for maintaining the Earth’s atmospheric oxygen content.
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Photosynthesis 3.5 thousand million years ago.

J M Olson1, B K Pierson

  • 1Institute of Biochemistry, Odense University, Campusvej 55, DK-5230, Odense M, Denmark.

Photosynthesis Research
|January 21, 2014
PubMed
Summary

Ancient life thrived 3.5 billion years ago, evidenced by stromatolites and microfossils. These early phototrophic prokaryotes likely used sulfur compounds for energy and were shielded from intense UV radiation by ferric iron in sediments.

Area of Science:

  • Origin of life studies
  • Paleobiology
  • Biogeochemistry

Background:

  • Stromatolites and microfossils in 3.5-billion-year-old rocks indicate early phototrophic prokaryotes.
  • Carbon isotope values suggest autotrophic CO2 fixation.
  • Sulfate deposits imply photosynthesis utilized reduced sulfur compounds.

Purpose of the Study:

  • To investigate the metabolic capabilities of early phototrophic prokaryotes.
  • To propose a mechanism for their survival under intense UV radiation in Earth's early atmosphere.

Main Methods:

  • Analysis of stromatolites and microfossils for evidence of early life.
  • Stable isotope analysis (δ(13)C) of sedimentary organic carbon.
  • Geochemical assessment of ancient sediment composition and UV-shielding properties.

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Main Results:

  • Evidence for phototrophic prokaryotes existing 3.5 billion years ago.
  • Autotrophic CO2 fixation and sulfur-based photosynthesis were likely.
  • Ancient photoautotrophs may have possessed single reaction centers with chlorophyll or bacteriochlorophyll and iron-sulfur centers.
  • Ferric iron in sediments likely provided UV shielding for submerged organisms.

Conclusions:

  • Phototrophic prokaryotes existed 3.5 billion years ago, utilizing CO2 fixation and sulfur compounds.
  • Abundant ferric iron in early sediments offered a protective UV shield, enabling survival.
  • Early photosynthesis likely involved chlorophyll or bacteriochlorophyll pigments.