Canon 350D Hap Griffin Baader Mod
46x180sec iso 1600
30 Darks/Flats/Bias
Celestron 9.25 reduced 0.63

Astroimaging Challenge Yahoo Group Runner-Up November, 2007

Discovered 1780 by Pierre Méchain, Messier 74 (M74, NGC 628) is one of the nicest examples of so-called "grand-design" spiral galaxies seen face-on, so that its spiral structure stands out conspicuously. With its comparatively low surface brightness, it is one of the more difficult objects in Messier's catalog, situated in constellation Pisces.

Its distance may be about 30 to 40 million light years, as it recedes with 793 km/sec. Its spiral arms are about 1000 light years broad. They are traced with clusters of blue young stars and pinkish colored diffuse gaseous nebulae (H II regions) in color photos, and reach out to cover a region of more than 10 minutes of arc in diameter, corresponding to roughly 95,000 light years, or about the same size as our Milky Way galaxy. The Webb Society deep sky observer's handbook gives a number of 193 known H II regions.

Two supernovae have been discovered in M74:

• Supernova 2002ap was discovered in M74 on January 29, 2002 by Japanese amateur Yoji Hirose when it was at mag 13.7. This type Ib/c supernova brightened up to mag 12.3 between February 5 and 12, 2002, and was classified as a "hypernova," occurring when progenitor stars of at least 40 solar masses explode.
• Supernova 2003gd was found visually in M74 by Bob Evans on June 12.82 UT, in the morning twilight at Australia as it was 13.2 mag bright, and already fading. This supernova was of type II.
  
  
  October 7, 2007