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Classifying Nebulae

For over a thousand years, astronomers wondered about the nature and development of nebulae. Nebulae appear to be faint clouds of gas and dust in the distant universe. Until recently, there have not been enough observations to classify nebulae based on their features or qualities.

During his studies of the spiral nebulae, Dr. Hubble proposed a system to classify all nebulae. He sorted them into three basic categories: elliptical, spiral, and irregular. These categories were further subdivided according to shape (spherical to elongated ellipses, for example) and structure (hazy to distinct spiral arms, barred spirals, etc.).

Hubble's system shows a sequence of evolutionary change but was "based primarily on the structural forms of photographic classification which should be entirely independent of theoretical considerations." Future astronomical studies and evidence will be the test for this new classification system. •

Images showing different classifications of galaxies
 		according to Hubble's classification scheme

Hubble's classification scheme

Image credit: NASA's Cosmic Times

Cosmic Times is a product of the Imagine the Universe! website. Imagine the Universe is a service of the High Energy Astrophysics Science Archive Research Center (HEASARC), Dr. Alan P. Smale (Director), within the Astrophysics Science Division (ASD) at NASA's Goddard Space Flight Center.

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Curator:Barbara Mattson
Responsible NASA Official:Phil Newman

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This page last updated: Wednesday, 24-Feb-2016 11:14:12 EST