M51 (Whirlpool Galaxy)
in Canes Venatici
The Whirlpool Galaxy, designated as M51, is a magnificent spiral galaxy located approximately 31 million light-years from Earth in the constellation Canes Venatici. This stunning celestial object is a quintessential example of a grand-design spiral galaxy, characterized by its remarkably well-defined and prominent spiral arms. The galaxy’s captivating appearance is largely due to its gravitational interaction with a smaller companion galaxy, NGC 5195, which is visibly tugging on one of M51’s outer arms. This interaction has triggered intense star formation within the Whirlpool Galaxy, illuminating its intricate structure with brilliant blue star clusters and pinkish nebulae. M51 was one of the first “nebulae” to be recognized as having a spiral structure, a discovery made by Lord Rosse in the mid-19th century, and it remains a favorite target for both professional astronomers and amateur stargazers due to its exquisite beauty and scientific significance. Written by Gemini.
Imaging Details
Telescope: 6 inch f/4 Newtonian with Paracorr Type 2 (effective focal length 690mm) and 2” Feather Touch Focuser
Camera: Player One Poseidon-C Pro, Anti-Halo Pro Ha+OIII filter, Phoenix Filter Wheel 2″x5
Resolution: 1.11 arcsec/px
Mount: Mesu Mount 200
Guiding: Player One OAG Max and ZWO ASI290MM Mini guide camera
Exposure Length: HOO: 300 sec x 60, OSC: 300 sec x 48
Location: Glenwood, MN
Date: 5/22/2025, 5/24/2025, 5/25/2025
Software: SciTech, SkyGuide (Innovations Foresight), N.I.N.A., Optic FocusLynx, Pixinsight, SkySafari Pro