Credit & Copyright: Yuri Beletsky
(ESO)
Explanation:
Is this a spiral galaxy?
No. Actually, it is the
Large Magellanic Cloud (LMC), the largest
satellite galaxy of our own
Milky Way Galaxy.
The LMC is
classified as a
dwarf irregular galaxy because of its normally chaotic appearance.
In this deep and wide exposure, however, the full extent of the
LMC becomes visible.
Surprisingly, during longer exposures, the
LMC begins to resemble a
barred spiral galaxy.
The
Large Magellanic Cloud lies only about 180,000
light-years
distant towards the constellation of
Dorado.
Spanning about 15,000 light-years, the LMC was the site of
SN1987A,
the brightest and closest
supernova
in modern times.
Together with the
Small Magellanic Cloud (SMC), the LMC can
be seen in Earth's southern hemisphere with the unaided
eye.
digg_url = 'http://apod.nasa.gov/apod/ap080409.html'; digg_skin = 'compact';
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A service of: LHEA at NASA / GSFC
& Michigan Tech. U.
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Publikacii s klyuchevymi slovami:
LMC - BMO - Bol'shoe Magellanovo Oblako
Publikacii so slovami: LMC - BMO - Bol'shoe Magellanovo Oblako | |
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