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  2. 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 ...

  3. HE 1523-0901 - Wikipedia

    en.wikipedia.org/wiki/HE_1523-0901

    HE 1523-0901 is the designation given to a red giant star in the Milky Way galaxy approximately 9,900 light-years from Earth. It is thought to be a second generation, Population II, or metal-poor, star ([Fe/H] = −2.95). The star was found in the sample of bright metal-poor halo stars from the Hamburg/ESO Survey by Anna Frebel and

  4. Stellar population - Wikipedia

    en.wikipedia.org/wiki/Stellar_population

    In reality, many population I stars are also found mixed in with the older population II stars. In 1944 , Walter Baade categorized groups of stars within the Milky Way into stellar populations . In the abstract of the article by Baade, he recognizes that Jan Oort originally conceived this type of classification in 1926 .

  5. Stellar evolution - Wikipedia

    en.wikipedia.org/wiki/Stellar_evolution

    Representative lifetimes of stars as a function of their masses The change in size with time of a Sun-like star Artist's depiction of the life cycle of a Sun-like star, starting as a main-sequence star at lower left then expanding through the subgiant and giant phases, until its outer envelope is expelled to form a planetary nebula at upper right Chart of stellar evolution

  6. K-type main-sequence star - Wikipedia

    en.wikipedia.org/wiki/K-type_main-sequence_star

    K-type main-sequence stars are about three to four times as abundant as G-type main-sequence stars, making planet searches easier. [17] K-type stars emit less total ultraviolet and other ionizing radiation than G-type stars like the Sun (which can damage DNA and thus hamper the emergence of nucleic acid based life). In fact, many peak in the red.

  7. Eureka, Missouri - Wikipedia

    en.wikipedia.org/wiki/Eureka,_Missouri

    Missouri Route 109 entering Eureka. The area's first known inhabitants were Shawnee Native Americans on the banks of the Meramec River; archaeological artifacts can still be found today as evidence of their past occupation of the area. [6] The village of Eureka was platted in 1858 [7] along the route of the Pacific Railroad. By 1890, the ...

  8. Category:Fire departments in Kentucky - Wikipedia

    en.wikipedia.org/wiki/Category:Fire_departments...

    Fire departments in the state of Kentucky, United States. Pages in category "Fire departments in Kentucky" The following 8 pages are in this category, out of 8 total.

  9. Stellar nucleosynthesis - Wikipedia

    en.wikipedia.org/wiki/Stellar_nucleosynthesis

    The first one, the proton–proton chain reaction, is the dominant energy source in stars with masses up to about the mass of the Sun. The second process, the carbon–nitrogen–oxygen cycle , which was also considered by Carl Friedrich von Weizsäcker in 1938, is more important in more massive main-sequence stars.