1843 stellar eruption may be new type of star explosion

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An artists conception of the fast blast wave from Eta Carinaes 1843 eruption which today has caught up with a slow-moving shell ejected in a previous outburst about 1000 years ago producing a bright fireworks display that heats the older shell and ma ...
An artist's conception of the fast blast wave from Eta Carinae's 1843 eruption, which today has caught up with a slow-moving shell ejected in a previous outburst about 1,000 years ago, producing a bright fireworks display that heats the older shell and makes it emit X-rays (orange). The well-known two-lobed "Homunculus" nebula, a slow-moving shell of gas and dust also produced in the 1843 eruption, is shown closer to the star, which is a hot blue supergiant. Credit: Gemini Observatory artwork by Lynette Cook

Eta Carinae, the galaxy's biggest, brightest and perhaps most studied star after the sun, has been keeping a secret: Its giant outbursts appear to be driven by an entirely new type of stellar explosion that is fainter than a typical supernova and does not destroy the star.


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All News summaries for September 10, 2008

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