NGC 1841 is a dense, ancient globular star cluster located in the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way, about 162,000 light-years away in the constellation Mensa. It's a "celestial fossil," containing very old stars that provide clues about early star formation, and is notable for being the southernmost globular cluster in the sky, visible from the Southern Hemisphere.
Type: Globular cluster, a tightly bound, spherical collection of hundreds of thousands of old stars.
Location: Within the Large Magellanic Cloud (LMC), a satellite galaxy of the Milky Way.
Distance: Approximately 162,000 light-years from Earth.
Constellation: Mensa.
Significance: Its ancient stars offer insights into the early universe and the formation of galaxies.
Visibility: Easily seen from the Southern Hemisphere with a telescope, as it's the southernmost globular cluster. Image Credit:
ESA/Hubble & NASA, A. Sarajedini, F. Niederhofer
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