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  2. Sheldon coin grading scale - Wikipedia

    en.wikipedia.org/wiki/Sheldon_coin_grading_scale

    Example of an Early American Cent - the coins that inspired Sheldon to create a more precise grading scale. (Courtesy of the National Numismatic Collection, National Museum of American History [photograph by Jaclyn Nash].) The Sheldon Coin Grading Scale is a 70-point coin grading scale used in the numismatic assessment of

  3. Logarithmic timeline - Wikipedia

    en.wikipedia.org/wiki/Logarithmic_timeline

    The present time is approximately 4.3 × 10 17 seconds after the Big Bang; the Sun and Earth formed about 2 × 10 17 seconds after the Big Bang. 10 20 seconds is 3 trillion years (3 × 10 12 years) in the future.

  4. Coin grading - Wikipedia

    en.wikipedia.org/wiki/Coin_grading

    Coin grading [1] is the process of determining the grade or condition of a coin, one of the key factors in determining its collectible value. A coin's grade is generally determined by six criteria: strike, preservation, luster, color, attractiveness, and occasionally the country/state in which it was minted. Several grading systems have been ...

  5. Category:Coin grading - Wikipedia

    en.wikipedia.org/wiki/Category:Coin_grading

    Sheldon coin grading scale; T. Third-party grading; V. VAM (Morgan and Peace dollar die varieties) ... This page was last edited on 6 August 2023, at 10:21 (UTC).

  6. Certified Acceptance Corporation - Wikipedia

    en.wikipedia.org/wiki/Certified_Acceptance...

    Grading standards have changed over the years. Because collectors and dealers have gotten more selective, an informal "sub-grade" system has evolved. "A" coins are the best of the grade, "B" coins are "solid", and "C" coins are at the low end of a particular grade based on the Sheldon scale, e.g., MS-65. CAC stickers are intended to standardize ...

  7. Photon epoch - Wikipedia

    en.wikipedia.org/wiki/Photon_epoch

    In physical cosmology, the photon epoch was the period in the evolution of the early universe in which photons dominated the energy of the universe. The photon epoch started after most leptons and anti-leptons were annihilated at the end of the lepton epoch, about 10 seconds after the Big Bang. [1]

  8. Cosmological decade - Wikipedia

    en.wikipedia.org/wiki/Cosmological_decade

    CÐ 100, the 100th cosmological decade, lasts from 10 100 to 10 101 seconds after Time Zero. CÐ is Time Zero. The epoch CÐ −43.2683 was 10 (−43.2683) seconds, which represents the Planck time since the Big Bang (Time Zero). There were an infinite number of cosmological decades between the Big Bang and the Planck epoch (or any other point ...

  9. Timeline of the universe - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_the_early_universe

    c. 10 −36 seconds: Electroweak epoch begins: The Universe cools down to 10 28 kelvin. The strong nuclear force becomes distinct from the electroweak force.; c. 10 −33 seconds: Space is subjected to inflation, expanding by a factor of the order of 10 26 over a time of the order of 10 −33 to 10 −32 seconds.