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  2. Cosmos Redshift 7 - Wikipedia

    en.wikipedia.org/wiki/Cosmos_Redshift_7

    Cosmos Redshift 7 (also known as COSMOS Redshift 7, Galaxy Cosmos Redshift 7, Galaxy CR7 or CR7) is a high-redshift Lyman-alpha emitter galaxy.At a redshift z = 6.6, [1] the galaxy is observed as it was about 800 million years after the Big Bang, during the epoch of reionisation. [1]

  3. Stellar population - Wikipedia

    en.wikipedia.org/wiki/Stellar_population

    By definition, each population group shows the trend where lower metal content indicates higher age of stars. Hence, the first stars in the universe (very low metal content) were deemed population III, old stars (low metallicity) as population II, and recent stars (high metallicity) as population I. [6] The Sun is considered population I, a ...

  4. HE 1327-2326 - Wikipedia

    en.wikipedia.org/wiki/HE_1327-2326

    HE 1327-2326, discovered in 2005 by Anna Frebel and collaborators, [2] was the star with the lowest known iron abundance until SMSS J031300.36−670839.3 was discovered. [5] The star is a member of Population II stars , with a solar-standardised iron to hydrogen index [Fe/H], or metallicity , of −5.4±0.2.

  5. Signal detected from 'cosmic dawn,' the birth of the first stars

    www.aol.com/article/news/2018/03/01/signal...

    The moment when the first stars in the universe lit up was detected by scientists this week in a revolutionary finding through a faint radio signal. Signal detected from 'cosmic dawn,' the birth ...

  6. SDSS J001820.5−093939.2 - Wikipedia

    en.wikipedia.org/wiki/SDSS_J001820.5%E2%88...

    This means that SDSS J0018−0939 most likely preserved the elemental abundance ratios produced by a first-generation very-massive star. [7] First generation stars are expected to self-regulate their growth by radiative feedback in the formation process, and to achieve masses typically tens of times that of the Sun. A fraction of stars might ...

  7. Chronology of the universe - Wikipedia

    en.wikipedia.org/wiki/Chronology_of_the_universe

    The first generation of stars, known as Population III stars, formed within a few hundred million years after the Big Bang. [58] These stars were the first source of visible light in the universe after recombination. Structures may have begun to emerge from around 150 million years, and early galaxies emerged from around 180 to 700 million years.

  8. Timeline of the early universe - Wikipedia

    en.wikipedia.org/wiki/Timeline_of_the_early_universe

    Because it is a Population II star, some suggestions have been raised that second generation star formation may have begun very early on. [7] The oldest-known star (confirmed) – SMSS J031300.36−670839.3, forms. 300 million years: First large-scale astronomical objects, protogalaxies and quasars may have begun forming.

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