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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. Trumpler 16 - Wikipedia

    en.wikipedia.org/wiki/Trumpler_16

    Trumpler 16 (Tr 16) is a massive open cluster that is home to some of the most luminous stars in the Milky Way galaxy. It is situated within the Carina Nebula complex in the Carina–Sagittarius Arm, located approximately 9,270 ly (2,842 pc) from Earth. [1]

  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. Gamma-ray burst - Wikipedia

    en.wikipedia.org/wiki/Gamma-ray_burst

    Eta Carinae, Apep, and WR 104 have been cited as possible future gamma-ray burst progenitors. [121] It is unclear if any star in the Milky Way has the appropriate characteristics to produce a gamma-ray burst. [122] The massive-star model probably does not explain all types of gamma-ray burst.

  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. ‘The Facts of Life’ Cast: Where Are They Now? - AOL

    www.aol.com/entertainment/facts-life-cast-where...

    More than 40 years after its premiere, The Facts of Life is still giving Us something to talk about. The sitcom debuted on NBC in August 1979 as a spinoff of Diff'rent Strokes. The Facts of Life ...

  9. Very Large Telescope - Wikipedia

    en.wikipedia.org/wiki/Very_Large_Telescope

    As of March 2008, the VLTI had already led to the publication of 89 peer-reviewed publications [68] and had published a first-ever image of the inner structure of the mysterious Eta Carinae. [69] In March 2011, the PIONIER instrument for the first time simultaneously combined the light of the four Unit Telescopes, potentially making VLTI the ...