Credit & Copyright: Ignacio
Diaz Bobillo
Explanation:
The
Tarantula Nebula is more than a thousand light-years in diameter,
a giant star forming region within nearby satellite galaxy the
Large Magellanic Cloud,
about 180 thousand light-years away.
The largest, most violent star forming region known in the whole Local
Group of galaxies, the cosmic arachnid sprawls across
this spectacular view
composed with narrowband data centered on emission
from ionized hydrogen and oxygen atoms.
Within the Tarantula (NGC 2070), intense radiation,
stellar winds and supernova shocks from the central young cluster of
massive stars, cataloged as R136,
energize the nebular glow and shape the spidery filaments.
Around
the Tarantula are other star forming regions with
young star clusters, filaments, and blown-out
bubble-shaped clouds.
In fact, the frame includes the site of the closest supernova in modern times,
SN 1987A,
right of center.
The rich field of view spans about 1 degree
or 2 full moons, in the southern
constellation
Dorado.
But were the Tarantula Nebula closer, say 1,500 light-years distant like
the local star forming Orion Nebula,
it would take up half the sky.
Watch:
Leonid Meteor Shower
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A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Publikacii s klyuchevymi slovami:
LMC - Tumannost' Tarantul - zvezdoobrazovanie - BMO - Bol'shoe Magellanovo Oblako
Publikacii so slovami: LMC - Tumannost' Tarantul - zvezdoobrazovanie - BMO - Bol'shoe Magellanovo Oblako | |
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