NGC5194 – the Whirlpool galaxy

in Canis Venatici

Info The Whirlpool Galaxy, also known as Messier 51a, M51a, and NGC 5194, is an interacting grand-design spiral galaxy with a Seyfert 2 active galactic nucleus. It lies in the constellation Canes Venatici, and was the first galaxy to be classified as a spiral galaxy. Its distance is 31 million light-years from Earth.  The galaxy and its companion, NGC 5195,are easily observed and the two galaxies may be seen with binoculars. The Whirlpool Galaxy has been extensively observed by professional astronomers, who study it to understand galaxy structure (particularly structure associated with the spiral arms) and galaxy interactions. hat later became known as the Whirlpool Galaxy was discovered on October 13, 1773, by Charles Messier while hunting for objects that could confuse comet hunters, and was designated in Messier’s catalogue as M51. Its companion galaxy, NGC 5195, was discovered in 1781 by Pierre Méchain, although it was not known whether it was interacting or merely another galaxy passing at a distance. However, the advent of radio astronomy and subsequent radio images of M51 unequivocally demonstrated that the Whirlpool and its companion galaxy are indeed interacting.  From Wikipedia.

Imaging Details

 

Telescope: 6 inch f/4 Newtonian with Paracorr Type 2 (effective focal length 690mm) and 2” Feather Touch Focuser
Camera: SBIG 8300C (3326 x 2504 pixels, 5.4 x 5.4µ); SBIG 8300M (3326 x 2504 pixels, 5.4 x 5.4µ)
FOV: ~1.49° x 1.12°
Mount: Mesu Mount 200
Guiding: Orion 60mm guidescope with helical focuser and ZWO ASI290MM Mini guide camera
Exposure Length: mono: 300 sec x 26; OSC: 300 sec x 35
Location: Glenwood, MN
Date: 6/30/2022, 7/1/2022
Software: SciTech, SkyGuide (Innovations Foresight), Sequence Generator Pro, Optic FocusLynx, Pixinsight, SkySafari Pro