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  2. Observable universe - Wikipedia

    en.wikipedia.org/wiki/Observable_universe

    So if the matter that originally emitted the oldest CMBR photons has a present distance of 46 billion light-years, then the distance would have been only about 42 million light-years at the time of decoupling. The light-travel distance to the edge of the observable universe is the age of the universe times the speed of light, 13.8 billion light ...

  3. Observational astronomy - Wikipedia

    en.wikipedia.org/wiki/Observational_astronomy

    The human eye discards what it sees from split-second to split-second, but photographic film gathers more and more light for as long as the shutter is open. The resulting image is permanent, so many astronomers can use the same data. It is possible to see objects as they change over time (SN 1987A is a spectacular example).

  4. Light-year - Wikipedia

    en.wikipedia.org/wiki/Light-year

    The light-month, roughly one-twelfth of a light-year, is also used occasionally for approximate measures. [37] [38] The Hayden Planetarium specifies the light month more precisely as 30 days of light travel time. [39] Light travels approximately one foot in a nanosecond; the term "light-foot" is sometimes used as an informal measure of time. [40]

  5. Time-domain astronomy - Wikipedia

    en.wikipedia.org/wiki/Time-domain_astronomy

    Light curve of NGC 2525 after a supernova. Time-domain astronomy is the study of how astronomical objects change with time. Said to have begun with Galileo's Letters on Sunspots, the field has now naturally expanded to encompass variable objects beyond the Solar System. Temporal variation may originate from movement of the source, or changes in ...

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

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

    2013 – The galaxy Z8 GND 5296 is confirmed by spectroscopy to be one of the most distant galaxies found up to this time. Formed just 700 million years after the Big Bang, expansion of the universe has carried it to its current location, about 13 billion light years away from Earth (30 billion light years comoving distance). [18]

  7. GN-z11 - Wikipedia

    en.wikipedia.org/wiki/GN-z11

    The object's name is derived from its location in the GOODS-North field of galaxies and its high cosmological redshift number (GN + z11). [12] It is observed as it existed 13.4 billion years ago, just 400 million years after the Big Bang ; [ 4 ] [ 13 ] [ 14 ] as a result, its distance is sometimes inappropriately [ 15 ] reported as 13.4 billion ...

  8. Cosmic time - Wikipedia

    en.wikipedia.org/wiki/Cosmic_time

    Cosmic time, or cosmological time, is the time coordinate commonly used in the Big Bang models of physical cosmology. [ 1 ] [ 2 ] This concept of time avoids some issues related to relativity by being defined within a solution to the equations of general relativity widely used in cosmology.

  9. Visual perception - Wikipedia

    en.wikipedia.org/wiki/Visual_perception

    [9] [10] He was the first person to explain that vision occurs when light bounces on an object and then is directed to one's eyes. [11] Leonardo da Vinci (1452–1519) is believed to be the first to recognize the special optical qualities of the eye. He wrote "The function of the human eye ... was described by a large number of authors in a ...