Triangulum Galaxy

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The Triangulum galaxy M33 is another prominent member of the Local Group of galaxies. This galaxy is small compared to its big apparent neighbor, the Andromeda galaxy M31, and to our Milky Way galaxy, but by this more of average size for spiral galaxies in the universe. One of the small Local Group member galaxies, LGS 3, is possibly a satellite of M33, which itself may be a remote but gravitationally bound companion of the Andromeda galaxy M31.

M33 was probably first found by Hodierna before 1654 (perhaps together with open cluster NGC 752). It was independently rediscovered by Charles Messier, and cataloged by him on August 25, 1764.

It is situated in the northeastern part of the galaxy; it has a diameter of nearly 1500 light years, and a spectrum similar to the Orion nebula M42. Over 200 young hot massive stars have recently formed here.



Photographs and astronomical descriptions courtesy of NASA and AURA/STScI


Tales of the Immortal Night ©2003, J.J. Kuhl

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