Dust lane

A dust lane is a relatively dense obscuring band of interstellar dust, observed as a dark swath against the background of a brighter object, especially a galaxy. These dust lanes can usually be seen in spiral galaxies (e.g., the Milky Way) when viewed from the edge. Due to the dense and relatively thick nature of this dust, light from the galaxy is reduced by several magnitudes. In the Milky Way, this reduction of light makes it impossible to see the light from the central bulge of the galaxy from Earth. This dust, as well as the gasses also found within these lanes, mix together and combine to form stars and planets.[1]

The Sombrero Galaxy features a prominent dust lane.

See also

References
  1. Sparke, L. S.; Gallagher, J. S. III (2007). Galaxies in the Universe. University Printing House, Cambridge CB2 *BS, United Kingdom: Cambridge University Press. ISBN 978-0-521-67186-6.CS1 maint: location (link)
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