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  2. Cosmological lithium problem - Wikipedia

    en.wikipedia.org/wiki/Cosmological_lithium_problem

    On the other hand, the Big Bang produced lithium-6 at levels more than 1000 times smaller. 7 4 Be later decayed via electron capture (half-life 53.22 days) into 7 3 Li, so that the observable primordial lithium abundance essentially sums primordial 7 3 Li and radiogenic lithium from the decay of 7 4 Be. These isotopes are produced by the reactions

  3. Lists of astronomical objects - Wikipedia

    en.wikipedia.org/wiki/Lists_of_astronomical_objects

    A black hole (artist concept); Vela Pulsar, a rotating neutron star; M80, a globular cluster, and the Pleiades, an open star cluster; The Whirlpool galaxy and Abell 2744, a galaxy cluster; Superclusters, galactic filaments and voids

  4. Stellar population - Wikipedia

    en.wikipedia.org/wiki/Stellar_population

    One possibility is that these stars were much larger than current stars: several hundred solar masses, and possibly up to 1,000 solar masses. Such stars would be very short-lived and last only 2–5 million years. [32] Such large stars may have been possible due to the lack of heavy elements and a much warmer interstellar medium from the Big Bang.

  5. Celestial spheres - Wikipedia

    en.wikipedia.org/wiki/Celestial_spheres

    In Greek antiquity the ideas of celestial spheres and rings first appeared in the cosmology of Anaximander in the early 6th century BC. [7] In his cosmology both the Sun and Moon are circular open vents in tubular rings of fire enclosed in tubes of condensed air; these rings constitute the rims of rotating chariot-like wheels pivoting on the Earth at their centre.

  6. Binary mass function - Wikipedia

    en.wikipedia.org/wiki/Binary_mass_function

    [5] [3] Using the mass function and the radial velocity of the host star, the minimum mass of an exoplanet can be determined. [ 15 ] [ 16 ] : 9 [ 12 ] [ 17 ] Applying this method on Proxima Centauri , the closest star to the solar system, led to the discovery of Proxima Centauri b , a terrestrial planet with a minimum mass of 1.27 M E .

  7. Orion's Belt - Wikipedia

    en.wikipedia.org/wiki/Orion's_Belt

    Orion's Belt is an asterism in the constellation of Orion.Other names include the Belt of Orion, the Three Kings, and the Three Sisters. [1] The belt consists of three bright and easily identifiable collinear star systems – Alnitak, Alnilam, and Mintaka – nearly equally spaced in a line, spanning an angular size of ~ 140′ (2.3°).

  8. Trapezium Cluster - Wikipedia

    en.wikipedia.org/wiki/Trapezium_Cluster

    The five brightest stars are on the order of 15 to 30 solar masses in size. They are within a diameter of 1.5 light-years of each other and are responsible for much of the illumination of the surrounding nebula. The Trapezium may be a sub-component of the larger Orion Nebula Cluster, a grouping of about 2,000 stars within a diameter of 20 light ...

  9. The Indestructibles - Wikipedia

    en.wikipedia.org/wiki/The_Indestructibles

    The Indestructibles (Ancient Egyptian: j.ḫmw-sk – literally "the ones not knowing destruction" [1] [2]) was the name given by ancient Egyptian astronomers to two bright stars which, at that time, could always be seen circling the North Pole. [3]