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  2. Eta Carinae - Wikipedia

    en.wikipedia.org/wiki/Eta_Carinae

    η Carinae (Eta Carinae, abbreviated to η Car), formerly known as η Argus, is a stellar system containing at least two stars with a combined luminosity greater than five million times that of the Sun, located around 7,500 light-years (2,300 parsecs) distant in the constellation Carina.

  3. Carina Nebula - Wikipedia

    en.wikipedia.org/wiki/Carina_Nebula

    The Cosmic Cliffs at the edge of NGC 3324, one of the first images taken by the James Webb Space Telescope. The Carina Nebula [7] or Eta Carinae Nebula [8] (catalogued as NGC 3372; also known as the Great Carina Nebula [9]) is a large, complex area of bright and dark nebulosity in the constellation Carina, located in the Carina–Sagittarius Arm of the Milky Way galaxy.

  4. Carina OB1 - Wikipedia

    en.wikipedia.org/wiki/Carina_OB1

    It includes the young star clusters Collinder 228, NGC 3293, NGC 3324, IC 2581, Trumpler 14, Trumpler 15 and Trumpler 16, [2] the last being the home of Eta Carinae. It also includes another massive and luminous star, HD 93129A. It is approximately 2,680 parsecs (8,700 ly) from Earth. [3]

  5. To match those observations, the models require much higher mass loss rates. Eta Carinae A has one of the highest known mass loss rates, currently around 10 −3 M ☉ /year, and is an obvious candidate for study. [95] Eta Carinae A is losing so much mass due to its extreme luminosity and relatively low surface gravity.

  6. Luminous blue variable - Wikipedia

    en.wikipedia.org/wiki/Luminous_blue_variable

    The most luminous are more than a million L ☉ (Eta Carinae reaches 4.6 million) and have masses approaching, possibly exceeding, 100 M ☉. The least luminous have luminosities around a quarter of a million L ☉ and masses as low as 10 M ☉ , although they would have been considerably more massive as main-sequence stars, due to their rapid ...

  7. HD 93205 - Wikipedia

    en.wikipedia.org/wiki/HD_93205

    HD 93205, or V560 Carinae, is a binary stellar system, in the Carina Nebula (NGC 3372) in the constellation Carina. It consists of two massive O-stars that revolve around each other in 6 days . The more massive member of the pair is an O3.5 main sequence star.

  8. Eta Carinids - Wikipedia

    en.wikipedia.org/wiki/Eta_Carinids

    The Eta Carinids are a meteor shower lasting from January 14 to 27 each year, peaking on January 21. C. S. Nilsson of the Adelaide Observatory discovered them in 1961 in Australia. [1] Roughly two to three meteors occur per hour at its maximum. [2] It gets its name from the radiant which is close to the stellar system Eta Carinae.

  9. List of statistical tests - Wikipedia

    en.wikipedia.org/wiki/List_of_statistical_tests

    Statistical tests are used to test the fit between a hypothesis and the data. [1] [2] Choosing the right statistical test is not a trivial task. [1]The choice of the test depends on many properties of the research question.

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