A nebular is a cloud of dust and gas inside a galaxy. Nebulae
become visible of the gas glows, or if the cloud reflects starlight or obscures
light from more distant objects. Emission nebulae shine because their gas emits
light when it is simulated by radiation from hot young stars. Reflection nebulae
shine because their dust reflects light from stars in or around the nebula.
Dark nebulae appear as silhouettes because they block out
light from shining nebulae or stars behind them. Two types of nebula are associated
with dying stars planetary nebulae and supernova remnants. Both consist of
expanding shells of gas that were once the outer layers of a star.
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