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  2. Cosmological horizon - Wikipedia

    en.wikipedia.org/wiki/Cosmological_horizon

    The particle horizon differs from the cosmic event horizon, in that the particle horizon represents the largest comoving distance from which light could have reached the observer by a specific time, while the cosmic event horizon is the largest comoving distance from which light emitted now can ever reach the observer in the future. [3]

  3. Fusa Miyake - Wikipedia

    en.wikipedia.org/wiki/Fusa_Miyake

    Cl produced by cosmic rays originating from the Sun when large solar flares or eruptions occur. Although the event was initially proposed to be a signature of an unidentified supernova, [2] it was soon independently confirmed and proven to be the discovery of an extreme solar particle event. [3] [4] The measurements utilised the 14

  4. Physical cosmology - Wikipedia

    en.wikipedia.org/wiki/Physical_cosmology

    Physical cosmology is a branch of cosmology concerned with the study of cosmological models. A cosmological model, or simply cosmology, provides a description of the largest-scale structures and dynamics of the universe and allows study of fundamental questions about its origin, structure, evolution, and ultimate fate. [1]

  5. List of future astronomical events - Wikipedia

    en.wikipedia.org/wiki/List_of_future...

    A METI message Cosmic Call 2 sent from the 70-metre Eupatoria Planetary Radar arrives at its destination, 55 Cancri. 2044 September Another METI message Cosmic Call 2 sent from the 70-metre Eupatoria Planetary Radar arrives at its destination, HD 10307. 2044 October 1 Occultation of Regulus by Venus. The last was on July 7, 1959, and the next ...

  6. Expansion of the universe - Wikipedia

    en.wikipedia.org/wiki/Expansion_of_the_universe

    Cosmic expansion is a key feature of Big Bang cosmology. It can be modeled mathematically with the Friedmann–Lemaître–Robertson–Walker metric (FLRW), where it corresponds to an increase in the scale of the spatial part of the universe's spacetime metric tensor (which governs the size and geometry of spacetime).

  7. Cosmological principle - Wikipedia

    en.wikipedia.org/wiki/Cosmological_principle

    In modern physical cosmology, the cosmological principle is the notion that the spatial distribution of matter in the universe is uniformly isotropic and homogeneous when viewed on a large enough scale, since the forces are expected to act equally throughout the universe on a large scale, and should, therefore, produce no observable inequalities in the large-scale structuring over the course ...

  8. Big History - Wikipedia

    en.wikipedia.org/wiki/Big_History

    Cosmic evolution, the scientific study of universal change, is closely related to Big History (as are the allied subjects of the epic of evolution and astrobiology); some researchers regard cosmic evolution as broader than Big History, since the latter mainly examines the specific historical trek from Big Bang → Milky Way → Sun → Earth ...

  9. Space weather - Wikipedia

    en.wikipedia.org/wiki/Space_weather

    The presence of cosmic rays in the near-Earth space environment can be detected by monitoring high-energy neutrons at ground level. Small fluxes of cosmic rays are present continuously. Large fluxes are produced by the Sun during events related to energetic solar flares. Total Electron Content (TEC) is a measure of the ionosphere over a given ...