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Messier 99

File:M99s_crop.jpg · Wikimedia Commons · See Wikimedia Commons

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Messier 99

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galaxy

AI overview

Messier 99 is a spiral galaxy located about 50 million light-years away in the constellation Coma Berenices. It's notable to astronomers as a well-studied example of a spiral galaxy and is bright enough to be observed through amateur telescopes.

AI-generated from the Wikipedia summary — may contain errors.

Wikidata facts

Distance from Earth
17
Image
M99s.jpg
Show 10 more facts
Commons category
Messier 99
catalog code
LEDA 39578
time of discovery or invention
1781-03-15
Commons gallery
Messier 99
redshift
0.008029
apparent magnitude
6.929
galaxy morphological type
Sc(dSc)
right ascension
184.7067708
declination
14.4164889
radial velocity
2399
Sources (5)

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Article

Messier 99 or M99, also known as NGC 4254 or St. Catherine's Wheel, is a grand design spiral galaxy in the northern constellation Coma Berenices approximately 15,000,000 parsecs (49,000,000 light-years) from the Milky Way. It was discovered by Pierre Méchain on 17 March 1781. The discovery was then reported to Charles Messier, who included the object in the Messier Catalogue of comet-like objects. It was one of the first galaxies in which a spiral pattern was seen. This pattern was first identified by Lord Rosse in the spring of 1846.

This galaxy has a morphological classification of SA(s)c, indicating a pure spiral shape with loosely wound arms. It has a peculiar shape with one normal looking arm and an extended arm that is less tightly wound. The galaxy is inclined by 42° to the line-of-sight with a major axis position angle of 68°.

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