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N11

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description N11 Overview

N11 is a large emission-nebula complex and H II region in the Large Magellanic Cloud, a satellite galaxy of the Milky Way. It is commonly described as the galaxy's second-largest star-forming region after the Tarantula Nebula and contains hot, young stars grouped in several OB associations. Stellar radiation and winds have ionized and reshaped the surrounding gas, producing shells, cavities, bright nebular arcs, and sites where additional star formation can be studied.

help N11 FAQ

Where is the N11 nebula located in the universe?

N11 is a massive H II region located in the Large Magellanic Cloud (LMC), which is a satellite galaxy of our Milky Way. It sits roughly 160,000 light-years away from Earth.

How does the N11 nebula compare in size to other objects in the Large Magellanic Cloud?

In the Large Magellanic Cloud, N11 is the second-largest nebula in terms of size and brightness. It is eclipsed only by the massive and highly famous 30 Doradus, commonly known as the Tarantula Nebula.

What kind of astronomical features can be found in N11?

The region is incredibly rich in OB associations, meaning it contains dense clusters of massive, hot, young stars. These bright stars emit intense ultraviolet radiation that ionizes the surrounding hydrogen gas, giving the nebula its glowing appearance.

Is N11 visible from Earth with a telescope?

Because the Large Magellanic Cloud is mostly visible from the Southern Hemisphere, N11 requires a southern sky to observe. It is too faint to see with the naked eye, but it can be captured in stunning detail by astrophotographers using moderate-to-large telescopes.

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