Messier 94

The Sab spiral galaxy M94 in the constellation Canes Venatici is considered by some (but not others) to be in a group including M64 and various fainter galaxies. It has an extremely bright innner region surrounded by a blue ring of young star clusters, then a fainter yellowish region of older stars also surrounded by traces of young stars, and even further out a very much fainter outer ring.

Although listed as a Spiral galaxy, through a 8" telescope, it appears as a slightly elliptical galaxy. In fact, it more closely resembles a small and compact globular cluster. The core is real bright, and quickly fading to nothingness.
You can find more information about this Messier object by visiting: SEDS - The Messier Catalog.


    M94
    NGC4736
    Dreyer description: Very bright, large, irregularly round, very abruptly very much brighter middle bright nucleus, resolvable, but mottled; = M94.
    Const: Canes Venatici
    Magnitude: 8.7
    RA: 12h 51m 06.9s Dec: +41°05'53"
    RA: 12h 50m 53.6s Dec: +41°07'10" (Epoch 2000)
    Azm: 58°10'31" Alt: +27°32'25"
    Rise: 09:02 Transit: 19:35 Set: 06:12
    Size:11.2' x 9.1'

RASC Charlottetown Centre