Timeline of cosmology

• 1576 - Thomas Digges[?] modifies the Copernican system by removing its outer edge and replacing the edge with a star-filled unbounded space
• 1610 - Johannes Kepler uses the dark night sky to argue for a finite universe
• 1720 - Edmund Halley puts forth an early form of Olbers' paradox
• 1744 - Jean-Phillipe de Cheseaux[?] puts forth an early form of Olbers' paradox
• 1826 - Heinrich Olbers puts forth Olbers' paradox
• 1917 - Willem de Sitter[?] derives an isotropic static cosmology with a cosmological constant as well as an empty expanding cosmology with a cosmological constant
• 1922 - Vesto Slipher[?] summarizes his findings on the spiral nebulae's systematic redshifts
• 1922 - Alexander Friedmann[?] finds a solution to the Einstein field equations[?] which suggests a general expansion of space
• 1927 - Georges Lemaître discusses the creation event of an expanding universe governed by the Einstein field equations
• 1928 - Harold Robertson[?] briefly mentions that Vesto Slipher's redshift measurements combined with brightness measurements of the same galaxies indicate a redshift-distance relation
• 1929 - Edwin Hubble demonstrates the linear redshift-distance relation and thus shows the expansion of the universe
• 1933 - Edward Milne[?] names and formalizes the cosmological principle
• 1934 - Georges Lemaître interprets the cosmological constant as due to a vacuum energy[?] with an unusual perfect fluid equation of state
• 1938 - Paul Dirac presents a cosmological theory where the gravitational constant decreases slowly so that the age of the universe divided by the atomic light-crossing time always equals the ratio of the electric force to the gravitational force between a proton and electron
• 1948 - Ralph Alpher[?], Hans Bethe, and George Gamow examine element synthesis in a rapidly expanding and cooling universe and suggest that the elements were produced by rapid neutron capture
• 1948 - Hermann Bondi[?], Thomas Gold, and Fred Hoyle propose steady state cosmologies based on the perfect cosmological principle
• 1951 - William McCrea shows that the steady state C-field can be accommodated within general relativity by interpreting it as a contribution to the energy-momentum tensor with an unusual equation of state
• 1961 - Robert Dicke[?] argues that carbon-based life can only arise when the Dirac large numbers hypothesis[?] is true because this is when burning stars exist; first use of the weak anthropic principle
• 1963 - Fred Hoyle and Jayant Narlikar[?] show that the steady state theory can explain the isotropy of the universe because deviations from isotropy and homogeneity exponentially decay in time
• 1964 - Fred Hoyle and Roger Tayler[?] point out that the primordial helium abundance depends on the number of neutrinos
• 1965 - Martin Rees[?] and Dennis Sciama[?] analyze quasar source count data and discover that the quasar density increases with redshift
• 1965 - Edward Harrison[?] resolves Olbers' paradox by noting the finite lifetime of stars
• 1966 - Stephen Hawking and George Ellis[?] show that any plausible general relativistic cosmology is singular
• 1966 - Jim Peebles[?] shows that the hot Big Bang predicts the correct helium abundance
• 1967 - Andrei Sakharov presents the requirements for a baryon-antibaryon asymmetry[?] in the universe
• 1967 - John Bahcall[?], Wal Sargent[?], and Maarten Schmidt[?] measure the fine-structure splitting of spectral lines in 3C191 and thereby show that the fine-structure constant does not vary significantly with time
• 1968 - Brandon Carter[?] speculates that perhaps the fundamental constants of nature must lie within a restricted range to allow the emergence of life; first use of the strong anthropic principle
• 1969 - Charles Misner[?] formally presents the Big Bang horizon problem
• 1969 - Robert Dicke[?] formally presents the Big Bang flatness problem
• 1973 - Edward Tryon[?] proposes that the universe may be a large scale quantum mechanical vacuum fluctuation where positive mass-energy is balanced by negative gravitational potential energy
• 1974 - Robert Wagoner[?], William Fowler[?], and Fred Hoyle show that the hot Big Bang predicts the correct deuterium and lithium abundances
• 1976 - A.I. Shlyakhter (http://alexonline.info) uses samarium ratios from the prehistoric natural fission reactor[?] in Gabon to show that some laws of physics have remained unchanged for over two billion years
• 1977 - Gary Steigman[?], David Schramm[?], and James Gunn[?] examine the relation between the primordial helium abundance and number of neutrinos and claim that at most five lepton families can exist
• 1980 - Alan Guth[?] proposes the inflationary Big Bang universe as a possible solution to the horizon and flatness problems
• 2003 - NASA's WMAP takes first detailed "baby picture" of the universe. The image reveals the universe is 13.7 billion years old (within one percent error) and that the inflationary theory is correct.