November 25, 2017

M43 (Nov. 2017)



Here is M43, the nebulosity surround in NU Orionis, the brightest star in this image.  NU Orionis is a B-type star and radiates UV radiation that probably makes M43 glow.

This image is just 16x240" through the CFF 290 Classical Cassegrain at eff. f/8.1 on a night of about average seeing, which means that 2453mm is too long for the seeing conditions.  It was shrunk 14% to accommodate the poor seeing conditions.  Still, it is an interesting image.  M43 is always overlooked for its near neighbor M42.

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