The Large Magellanic Cloud (LMC) is a dwarf satellite galaxy of the Milky Way, located about 160,000–200,000 light‑years away in the southern constellations Dorado and Mensa. Roughly 10,000 light‑years across, it is rich in star-forming regions—such as the Tarantula Nebula—and contains billions of stars.
Image Credit:
Anglo-Australian Telescope
Board
Explanation:
Magellan and his crew had plenty of time to study the southern sky
during their famous voyage around the world. As a result, two fuzzy
cloud like objects, nestled among the southern constellations of Doradus
and Tucana are now
known as the Clouds of Magellan. The Magellanic Clouds are small irregular
galaxies, satellites of our
larger Milky Way spiral galaxy.
The Large Magellanic Cloud
(LMC) pictured above is the closest galaxy to our own Milky Way,
at a distance of about 180,000 light years.
The Magellanic Clouds are joined to the Milky Way by a
stream of cold hydrogen gas whose origin is still controversial.
An unusual effect called
gravitational lensing has recently
been detected in a few LMC stars, and there is hope this could
tell us important information about the
true composition of our universe.
Tomorrow's picture: The Small Cloud of Magellan
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Astronomy Picture of the Day (TM) is created and copyrighted in 1995 by
Robert
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Jerry
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/ NASA APOD
Magellan and his crew had plenty of time to study the southern sky during their famous voyage around the world. As a result, two fuzzy cloud like objects, nestled among the southern constellations of Doradus and Tucana are now known as the Clouds of Magellan. The Magellanic Clouds are small irregular galaxies, satellites of our larger Milky Way spiral galaxy. The Large Magellanic Cloud (LMC) pictured above is the closest galaxy to our own Milky Way, at a distance of about 180,000 light years. The Magellanic Clouds are joined to the Milky Way by a stream of cold hydrogen gas whose origin is still controversial. An unusual effect called gravitational lensing has recently been detected in a few LMC stars, and there is hope this could tell us important information about the true composition of our universe.