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  2. Chunithm - Wikipedia

    en.wikipedia.org/wiki/Chunithm

    Chunithm [2] (stylized in all caps) is an arcade rhythm game developed and published by Sega.It was first seen in select Japanese arcades in November 2014, as part of a location test [3] [4] and was officially released on July 16, 2015 (). [5]

  3. List of most luminous stars - Wikipedia

    en.wikipedia.org/wiki/List_of_most_luminous_stars

    The last stars in the list are familiar nearby stars put there for comparison, and not among the most luminous known. It may also interest the reader to know that the Sun is more luminous than approximately 95% of all known stars in the local neighbourhood (out to, say, a few hundred light years), due to enormous numbers of somewhat less ...

  4. O-type main-sequence star - Wikipedia

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

    An O-type main-sequence star (O V) is a main-sequence (core hydrogen-burning) star of spectral type O and luminosity class V. These stars have between 15 and 90 times the mass of the Sun and surface temperatures between 30,000 and 50,000 K. They are between 40,000 and 1,000,000 times as luminous as the Sun.

  5. List of nearest bright stars - Wikipedia

    en.wikipedia.org/wiki/List_of_nearest_bright_stars

    Prominent stars in the neighborhood of the Sun (center) This list of nearest bright stars is a table of stars found within 15 parsecs (48.9 light-years) of the nearest star, the Sun, that have an absolute magnitude of +8.5 or brighter, which is approximately comparable to a listing of stars more luminous than a red dwarf.

  6. File:Star*.svg - Wikipedia

    en.wikipedia.org/wiki/File:Star*.svg

    A golden star. See also Image:Star.svg. File usage. More than 100 pages use this file. The following list shows the first 100 pages that use this file only.

  7. Rho Cassiopeiae - Wikipedia

    en.wikipedia.org/wiki/Rho_Cassiopeiae

    Rho Cassiopeiae (/ ˌ r oʊ k æ s i ə ˈ p iː aɪ,-s i oʊ-,-iː /; ρ Cas, ρ Cassiopeiae) is a yellow hypergiant star in the constellation Cassiopeia.It is about 8,150 light-years (2,500 pc) from Earth, yet can still be seen by the naked eye as it is over 300,000 times brighter than the Sun.

  8. Hayashi track - Wikipedia

    en.wikipedia.org/wiki/Hayashi_track

    While slowly contracting, the star follows the Hayashi track downwards, becoming several times less luminous but staying at roughly the same surface temperature, until either a radiative zone develops, at which point the star starts following the Henyey track, or nuclear fusion begins, marking its entry onto the main sequence.

  9. List of luminous blue variable stars - Wikipedia

    en.wikipedia.org/wiki/List_of_Luminous_Blue...

    Star system Nebula Median distance Stars in system Spectral type Apparent magnitude (V) Comments and references P Cygni (34 Cygni) 5251±180: 1: B1-2 Ia-0ep: 4.82: The closest luminous blue variable star to Earth V4029 Sagittarii (HD 168607) 6,000 1 B9Ia + 8.12 to 8.29 [4] [5] near the Omega Nebula: V905 Scorpii (HD 160529) 6,100 1 LBV 6.66 [4] [5]

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