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Last updated April 11, 2025

Hydrogen (Z=1): The Key to Cosmic Creation

Structure of the hydrogen atom

In the Beginning, There Was Hydrogen

Hydrogen (symbol H, atomic number 1) is the simplest, lightest, and most abundant chemical element in the universe. It plays a fundamental role in fundamental physics, astrophysics, chemistry, and engineering.

Contribution of Hydrogen to Vital Processes

Hydrogen, mainly in the form of H⁺ (protons) and bonded within organic molecules, plays a fundamental role in cellular bioenergetics. It is involved in the electron transport chain (Krebs cycle and oxidative phosphorylation), where proton gradients across mitochondrial membranes drive ATP synthesis. It also contributes to intracellular pH regulation and numerous enzymatic reactions (notably redox reactions). Consequence of a deficiency: An imbalance in H⁺ quickly disrupts energy metabolism, acid–base equilibrium, and protein stability, potentially leading to severe cellular failure or cell death.

History of Discovery

17th Century: First Observations
Hydrogen gas was first observed by Théodore de Mayerne (1605) and then by Robert Boyle (1660), when they noticed that a metal reacting with an acid produced a flammable gas, without identifying it as a distinct element.

1766: Identification by Henry Cavendish
Henry Cavendish isolated and studied this gas, which he named "inflammable air." He demonstrated that its combustion produced water, contradicting the idea that water was an element.

1783: Naming by Antoine Lavoisier
Lavoisier established that water is a compound of two gases: hydrogen and oxygen. He gave the gas the name "hydrogen," from the Greek hydro (water) and genes (generate).

Atomic Structure

Constitution: One proton and one electron, no neutron for the most common isotope (¹H, protium).
Isotopes:

Physical Properties

Chemical Reactivity

Industrial and Technological Applications

Cosmological and Astrophysical Role

Fundamental Physical Issues

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