M51 with Super Nova
M51 with Supernova
July 1, 2005
Takahashi Epsilon 210 Astrograph
SBIG STL 11000 Camera
30 Minutes Luminance; R15, G10, B15 Binned 2x2
The Supernova is the 'star' closest to the center of the nucleus of the main galaxy in this image.
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