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Messier 77 (NGC1068)

Messier 77 (NGC1068) Spiral Galaxy in Cetus

Messier 77 (NGC1068) is a spiral galaxy object of interest in space. It lies at a distance of 47000000 light years away in the constellation of Cetus.

It is referred to as M(77) when it was catalogued by Charles Messier in 18th - 19th Century France. It is also referred to as NGC(1068) 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 Spiral Galaxy's location is 02:42.7 (R.A.) and -00:01 (Dec.). Its Visual Brightness is a 8.9 Magnitude and has an apparent magnitude of 10.00000 with an apparent dimension of 7x6 . The object can not be seen by the naked eye, you need a telescope to see it.

(M77,NGC1068) is a spiral galaxy. It was discovered in 1780 by Pierre Mechain. It's location is RA(02:42.7), Dec(-00:01) and its distance is calculated 47000 light years away. Its visual Brightness is 8.9. Its apparent dimensions measured in arcmins is 7x6.

Fact File

NameMessier 77 (NGC1068)
TypeSpiral Galaxy
Messier Id77
NGC Id1068
Right Ascension02:42.7
Distance (Lt.Yr)47000000
Visual Brightness8.9
Apparent Dimension7x6
Apparent Magnitude10.00000
Naked Eye VisibleRequires a 7x50 Binoculars - Magnitudes
Year of Discovery1780
DiscovererPierre Mechain

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