Posted on 04/10/2003 6:03:50 AM PDT by petuniasevan
Discover the cosmos! Each day a different image or photograph of our fascinating universe is featured, along with a brief explanation written by a professional astronomer.
Explanation: Blossoming in nearby galaxy the Large Magellanic Cloud (LMC), this gorgeous nebula is energized by radiation and winds from a massive star whose surface temperature approaches 100,000 degrees. The composite color image from the European Southern Observatory's Melipal telescope resolves details in the energetic nebula, with emission from helium atoms in blue hues, oxygen atoms in green, and hydrogen atoms in red. While emission nebulae generally show the familiar red light from ionized hydrogen atoms - hydrogen atoms with their electrons stripped away - ionized helium atoms are tracers of even higher energy interactions. The intriguing filaments of helium emission make this and other recently studied emission nebulae most exceptional. A Wolf-Rayet star, the massive star powering this nebula, created a cosmic bubble with stellar winds in the early stages of its life. Part of the bubble is still apparent as the large arc in the lower portion of the image. The area pictured is about 150 light-years across.
The LMC is located in the southern hemisphere constellation of Dorado. It isn't visible from north of 20 degrees north latitude.
The Wolf-Rayet star which powers the nebula (BAT99-2) is an object for large telescopes at magnitude 16.22 visual.
The LMC is our largest satellite galaxy, and second in proximity only to the Small Magellanic Cloud.
The supernova 1987A occurred in the LMC. Here's a Hubble image of the very intriguing aftermath:
See this Supernova Remnant in detail as well as the Crab SNR and Tycho's Star SNR at this link: Astronomy Picture of the Day Index - Nebulae: Supernova Remnants
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