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  2. Edwin Hubble - Wikipedia

    en.wikipedia.org/wiki/Edwin_Hubble

    Edwin Powell Hubble (November 20, 1889 – September 28, 1953) [1] was an American astronomer. He played a crucial role in establishing the fields of extragalactic astronomy and observational cosmology .

  3. C/1937 P1 (Hubble) - Wikipedia

    en.wikipedia.org/wiki/C/1937_P1_(Hubble)

    Comet Hubble, formally designated C/1937 P1, is the first and only comet discovered by astronomer Edwin Hubble. The comet was already on its outbound flight when it was first spotted in August 1937 as a magnitude 13.5 object in the constellation Sagittarius. [1] [5] It is the fourth comet discovered in 1937. [6]

  4. Hubble's law - Wikipedia

    en.wikipedia.org/wiki/Hubble's_law

    A closed universe with Ω M > 1 and Ω Λ = 0 comes to an end in a Big Crunch and is considerably younger than its Hubble age. An open universe with Ω M ≤ 1 and Ω Λ = 0 expands forever and has an age that is closer to its Hubble age. For the accelerating universe with nonzero Ω Λ that we inhabit, the age of the universe is coincidentally ...

  5. Timeline of astronomy - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_astronomy

    Edwin Hubble discovered that the universe is expanding and that the farther away a galaxy is, the faster it is moving away from us. Two years later, Georges Lemaître suggests that the expansion can be traced to an initial "Big Bang".

  6. History of the Big Bang theory - Wikipedia

    en.wikipedia.org/wiki/History_of_the_Big_Bang_theory

    Hubble's idea allowed for two opposing hypotheses to be suggested. One was Lemaître's Big Bang, advocated and developed by George Gamow. The other model was Fred Hoyle's steady-state model, in which new matter would be created as the galaxies moved away from each other. In this model, the universe is roughly the same at any point in time.

  7. Observational cosmology - Wikipedia

    en.wikipedia.org/wiki/Observational_cosmology

    In the 1970s numerous studies showed that tiny deviations from isotropy in the CMB could result from events in the early universe. [33]: 8.5.1 Harrison, [34] Peebles and Yu, [35] and Zel'dovich [36] realized that the early universe would require quantum inhomogeneities that would result in temperature anisotropy at the level of 10 −4 or 10 −5.

  8. Cosmic age problem - Wikipedia

    en.wikipedia.org/wiki/Cosmic_age_problem

    Following theoretical developments of the Friedmann equations by Alexander Friedmann and Georges Lemaître in the 1920s, and the discovery of the expanding universe by Edwin Hubble in 1929, it was immediately clear that tracing this expansion backwards in time predicts that the universe had almost zero size at a finite time in the past.

  9. Timeline of knowledge about galaxies, clusters of galaxies ...

    en.wikipedia.org/wiki/Timeline_of_knowledge...

    1998 – The Hubble Deep Field South is compiled. 1998 – Discovery of accelerating universe. [13] 2000 – Data from several cosmic microwave background experiments give strong evidence that the Universe is "flat" (space is not curved, although space-time is), with important implications for the formation of large-scale structure.