Astronomer who first proposed the existence of dark matter based on galaxy cluster motions.Fritz Zwicky was a Swiss astronomer who, in 1933, made the first compelling observation that led to the concept of dark matter. While studying the Coma galaxy cluster, he noticed that the galaxies were moving so fast that the cluster should have flown apart if only visible matter were present. He proposed that an unseen 'dark matter' must be providing the extra gravitational pull to hold the cluster together. This idea was initially met with skepticism but has since become a cornerstone of modern cosmology.
Fritz Zwicky introduced the dark matter hypothesis in 1933 based on his observations of the Coma cluster. His work was largely ignored for decades until the 1970s when Vera Rubin's studies of galaxy rotation curves provided further evidence.
Zwicky applied the virial theorem, which relates the average kinetic energy of a system to its gravitational potential energy, to estimate the total mass of the Coma cluster. He found that the mass required to keep the cluster bound was about 400 times greater than what could be accounted for by the luminous galaxies. This discrepancy implied the existence of a large amount of non-luminous matter. Modern observations, such as gravitational lensing and cosmic microwave background measurements, confirm that about 27% of the universe's energy density is dark matter, though its exact nature remains unknown.
The concept of dark matter is crucial for interpreting astronomical observations and for developing cosmological models, such as the Lambda-CDM model, which describes the evolution of the universe from the Big Bang to the present.
Zwicky was also the first to propose the existence of neutron stars and was a pioneer in the search for supernovae, discovering many himself by systematically scanning galaxies with a telescope.









