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Acknowledgements
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Universe of the Hubble Space Telescope
2000 Calendar
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| N 81 is a glowing nebula of gas, dust, and stars
located some 200,000 light years away in the Small Magellanic
Cloud, a companion galaxy of the Milky Way galaxy visible in
the skies of the Southern Hemisphere. The nebula is a site of
massive star formation, and more than 50 individual stars can
be identified within the core of the nebula, which spans only
10 light years in diameter. The orange glow of the nebula is
produced as ultraviolet light from the young, hot, massive stars
is absorbed by the gas and re-radiated at visible wavelengths. |
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