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M 94

Spiral Galaxy M94 (NGC 4736), type Sb, in Canes Venatici

Right Ascension 12 : 50.9 (h:m)
Declination +41 : 07 (deg:m)
Distance 14500 (kly)
Visual Brightness 8.2 (mag)
Apparent Dimension 7x3 (arc min)

Discovered by Pierre Méchain in 1781.

Spiral galaxy M94 was classified Sab because of its extremely bright inner region (overexposed in our image). This bright circular disk is surrounded by a ring of active star-forming regions, traced by blue young star clusters in color images, which sharply separates it from a much less bright outer ring of an older yellowish stellar population. In the outskirts, this region however ends again in a ring with moderate star formation activity, so that M94 is one of the relatively rare galaxies in which two "waves" of stellar formation can be observed. In very long exposures, a further very faint ring, about 15 arc minutes across, becomes visible, a suggestion of which is visible in the DSSM image of M94, but see also the inset in the Hubble Atlas of Galaxies.

The distance of M94 is not yet well-determined (at least to the knowledge of the present author). Tully gives about 14 million light years, Burnham 20, Kenneth Glyn Jones 33 million light years.

  • Historical Observations and Descriptions of M94
  • More images of M94
  • Astro-2 images of M94 (Space Shuttle mission STS-67)
  • Amateur images of M94

  • Multispectral Image Collection of M94, SIRTF Multiwavelength Messier Museum

  • SIMBAD Data of M94
  • NED Data of M94
  • Observing Reports for M94 (IAAC Netastrocatalog)

    Hartmut Frommert (spider@seds.org)
    Christine Kronberg (smil@lrz.uni-muenchen.de)

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    Last Modification: 9 Dec 1999, 22:59 MET