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This timeline of cosmological theories and discoveries is a chronological catalog of the evolution of humankind's understanding of the cosmos over the last two-plus millennia. Modern cosmological conceptions follow the development of the scientific discipline of physical cosmology.
[edit] Pre-1900
- 8th century BCE- Yajnavalkya proposes a lunisolar cycle and was attributed other heliocentric ideas
- 3rd century BCE- Aristarchus of Samos proposes a Sun-centered Universe
- 2nd century CE - Ptolemy proposes an Earth-centred Universe, with the Sun and planets revolving around the Earth
- 5th-16th centuries - Several astronomers propose a Sun-centered Universe, including Aryabhata, Bhaskara I, Ibn al-Shatir, and Copernicus
- 1576 - Thomas Digges modifies the Copernican system by removing its outer edge and replacing the edge with a star-filled unbounded space
- 1584 - Giordano Bruno proposes a non-hierarchical cosmology, wherein the Copernican solar system is not the centre of the universe, but rather, a relatively insignificant star system, amongst an infinite multitude of others
- 1610 - Johannes Kepler uses the dark night sky to argue for a finite universe
- 1687 - Sir Isaac Newton's laws describe large-scale motion throughout the universe
- 1720 - Edmund Halley puts forth an early form of Olbers' paradox
- 1744 - Jean-Philippe de Cheseaux puts forth an early form of Olbers' paradox
- 1791 - Erasmus Darwin pens the first description of a cyclical expanding and contracting universe in his poem The Economy of Vegetation
- 1826 - Heinrich Wilhelm Olbers puts forth Olbers' paradox
- 1848 - Edgar Allan Poe offers first correct solution to Olbers' paradox in Eureka: A Prose Poem, an essay that also suggests the expansion and collapse of the universe
[edit] 1900-1949
- 1905 - Albert Einstein publishes the Special Theory of Relativity, positing that space and time are not separate continua
- 1915 - Albert Einstein publishes the General Theory of Relativity, showing that an energy density warps spacetime
- 1917 - Willem de Sitter derives an isotropic static cosmology with a cosmological constant, as well as an empty expanding cosmology with a cosmological constant, termed a de Sitter universe
- 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 - Howard Percy 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 suggests the large numbers hypothesis, that the gravitational constant may be small because it is decreasing slowly with time
- 1948 - Ralph Alpher, Hans Bethe ("in absentia"), 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
- 1948 - George Gamow predicts the existence of the cosmic microwave background radiation by considering the behavior of primordial radiation in an expanding universe
[edit] 1950 to 1999
- 1950 - Fred Hoyle derisively coins the term "Big Bang".
- 1961 - Robert Dicke argues that carbon-based life can only arise when the gravitational force is small, because this is when burning stars exist; first use of the weak anthropic principle
- 1965 - Hannes Alfvén proposes the now-discounted concept of ambiplasma to explain baryon asymmetry.
- 1965 - Martin Rees and Dennis Sciama analyze quasar source count data and discover that the quasar density increases with redshift.
- 1965 - Arno Penzias and Robert Wilson, astronomers at Bell Labs discover the 2.7 K microwave background radiation, which earns them the 1978 Nobel Prize in Physics. Robert Dicke, James Peebles, Peter Roll and David Todd Wilkinson interpret it as relic from the big bang.
- 1966 - Stephen Hawking and George Ellis show that any plausible general relativistic cosmology is singular
- 1966 - James Peebles shows that the hot Big Bang predicts the correct helium abundance
- 1967 - Andrei Sakharov presents the requirements for baryogenesis, 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 - Alex Shlyakhter uses samarium ratios from the Oklo prehistoric natural nuclear 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.
- 1981 - Viacheslav Mukhanov and G. Chibisov propose that quantum fluctuations could lead to large scale structure in an inflationary universe
- 1981 - Alan Guth proposes the inflationary Big Bang universe as a possible solution to the horizon and flatness problems
- 1990 - Preliminary results from NASA's COBE mission confirm the cosmic microwave background radiation is an isotropic blackbody to an astonishing one part in 105 precision, thus eliminating the possibility of an integrated starlight model proposed for the background by steady state enthusiasts.
- 1990s - Ground based cosmic microwave background experiments measure the first peak, determine that the universe is geometrically flat.
- 1998 - Controversial evidence for the fine structure constant varying over the lifetime of the universe is first published.
- 1998 - Adam Riess, Saul Perlmutter and others discover the cosmic acceleration in observations of Type Ia supernovae providing the first evidence for a non-zero cosmological constant.
- 1999 - Measurements of the cosmic microwave background radiation (most notably by the BOOMERanG experiment see Mauskopf et al., 1999, Melchiorri et al., 1999, de Bernardis et al. 2000) provide evidence for oscillations (peaks) in the anisotropy angular spectrum as expected in the standard model of cosmological structure formation. These results indicates that the geometry of the universe is flat. Together with large scale structure data, this provides complementary evidence for a non-zero cosmological constant.
[edit] Since 2000
- 2006 - The long-awaited three-year WMAP results are released, confirming previous analysis, correcting several points, and including polarization data.
[edit] See also
[edit] References
- Bunch, Bryan, and Alexander Hellemans, "The History of Science and Technology: A Browser's Guide to the Great Discoveries, Inventions, and the People Who Made Them from the Dawn of Time to Today". ISBN 0-618-22123-9
- P. Mauskopf et al.,astro-ph/9911444, Astrophys.J. 536 (2000) L59-L62.
- A. Melchiorri et al.,astro-ph/9911445, Astrophys.J. 536 (2000) L63-L66.
- P. de Bernardis et al., astro-ph/0004404, Nature 404 (2000) 955-959.
