1938Hans Bethe Explains Stellar Energy Generation

German physicist Hans Bethe explains how stars generate ener...
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Year
1920
1938
1939

🌟 Eddington proposes stellar nucleosynthesis

Eddington proposes stellar nucleosynthesis (1920)
Stellar NucleosynthesisAstrophysicsEddingtonNuclear PhysicsCosmologyStars20th Century
United KingdomUnited Kingdom

🌟 Hans Bethe Explains Stellar Energy Generation

German physicist Hans Bethe explains how stars generate energy. He outlines a series of nuclear fusion reactions that turn hydrogen into helium and release enormous amounts of energy in a star's core. These reactions use the star's hydrogen very slowly, allowing it to burn for billions of years.
Hans Bethe Explains Stellar Energy Generation (1938)
AstrophysicsNuclear PhysicsStellar NucleosynthesisNuclear FusionHans BetheEnergy ProductionStars1930s
GermanyGermany

⚛️ Isidor Rabi: Nuclear Magnetic Resonance

Isidor Rabi: Nuclear Magnetic Resonance (1938)
Nuclear PhysicsSpectroscopyIsidor RabiMagnetic ResonanceQuantum MechanicsMolecular Physics1930sPhysics
United StatesUnited States

☢️ Otto Hahn, Lise Meitner and Fritz Strassmann: Nuclear Fission Discovered

Otto Hahn, Lise Meitner and Fritz Strassmann: Nuclear Fission Discovered (1938)
Nuclear PhysicsNuclear FissionOtto HahnLise MeitnerFritz StrassmannRadioactivityAtomic Energy1930sHeavy Nuclei
GermanyGermany

🌟 Stellar Fusion Explains Energy Production in Stars

39 – Stellar fusion explains energy production in stars
Stellar Fusion Explains Energy Production in Stars (1938)
AstrophysicsNuclear PhysicsStellar NucleosynthesisNuclear FusionHans BetheEnergy ProductionStars1930s
GermanyGermany

☢️ Otto Hahn and Lise Meitner Discover the Process of Nuclear Fission in Uranium

Otto Hahn and Lise Meitner discover the process of nuclear fission in uranium.
Otto Hahn and Lise Meitner Discover the Process of Nuclear Fission in Uranium (1939)
Nuclear PhysicsNuclear FissionOtto HahnLise MeitnerRadioactivityAtomic EnergyUranium1930s
GermanyGermanySwedenSweden