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The Triangulum Galaxy (M33, NGC598)

The Triangulum Galaxy is a spiral galaxy object of interest in space. It lies at a distance of 2,380-3,070 kly light years away in the constellation of Triangulum. It is referred to as M(33) when it was catalogued by Charles Messier in 18th - 19th Century France. It is referred to as NGC(598) in the New General Catalogue. This is a list of deep space objects that was compiled by John Louis Emil Dreyer in 1888 in an update to John Herschel earlier catalogue. The Triangulum Galaxy was discovered in 1764 by Charles Messier. The Spiral Galaxy's location is 01:33.9 (R.A.) and +30:39 (Dec.). Its Visual Brightness is a 5.7 Magnitude and has an apparent magnitude of 6 with an apparent dimension of 73x45 .

The Triangulum Galaxy (M33,NGC598) is a spiral galaxy. It was discovered in 1764 by Charles Messier. It's location is RA(01:33.9), Dec(+30:39) and its distance is calculated 2.380-3.070 million light years away. Its visual Brightness is 5.7. Its apparent dimensions measured in arcmins is 73x45.

The Triangulum Galaxy does not get its name from its shape, its name is from the constellation that it can be located in, Triangulum. It is a local galaxy and will one day along with the Andromeda Galaxy collide into our Milky Way. The good news is that it won't happens billions of years, long after we've gone.

Although it is small compared to IC 1101 galaxy, it has a number of new star forming areas and will carry on for a long time yet. The galaxy was one of three galaxies that appeared in the television series Andromeda along with the milky way and the Andromeda Galaxy.

Fact File

NameThe Triangulum Galaxy
TypeSpiral Galaxy
Messier Id33
NGC Id598
TypeSpiral Galaxy
Right Ascension01:33.9
Distance (Lt.Yr)2,380-3,070 kly
Visual Brightness5.7
Apparent Dimension73x45
Apparent Magnitude6
Year of Discovery1764
DiscovererCharles Messier
CoprightAnglo-Australian Observatory

The Triangulum Galaxy (M33, NGC598) Spiral Galaxy in Triangulum

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