NGC2841 - Spiral Galaxy in Ursa Major

ngc2841 in LRGB

ngc2841 - Spiral Galaxy in Ursa Major

From Wikipedia:

NGC 2841 is an unbarred spiral galaxy in the northern circumpolar constellation of Ursa Major. It was discovered on 9 March 1788 by German-born astronomer William Herschel. J. L. E. Dreyer, the author of the New General Catalogue, described it as, "very bright, large, very much extended 151, very suddenly much brighter middle equal to 10th magnitude star". Initially thought to be about 30 million light-years distant, a 2001 Hubble Space Telescope survey of the galaxy's Cepheid variables determined its distance to be approximately 14.1 megaparsecs or 46 million light-years. The optical size of the galaxy is 8.′1 3.′5.

This is the prototype for the flocculent spiral galaxy, a type of spiral galaxy whose arms are patchy and discontinuous. The morphological class is SAa, indicating a spiral galaxy with no central bar and very tightly-wound arms. There is no grand design structure visible in the optical band, although some inner spiral arms can be seen in the near infrared. It is inclined by an angle of 68 to the line of sight from the Earth, with the major axis aligned along a position angle of 148.

The properties of NGC 2841 are similar to those of the Andromeda Galaxy. It is home to a large population of young blue stars, and a few H II regions. The luminosity of the galaxy is 21010 L☉ and it has a combined mass of 71010 M☉. Its disk of stars can be traced out to a radius of around 228 kly (70 kpc). This disk begins to warp at a radius of around 98 kly (30 kpc), suggesting the perturbing effect of in-falling matter from the surrounding medium.

The rotational behavior of the galaxy suggests there is a massive nuclear bulge, with a low-ionization nuclear emission-line region (LINER) at the core; a type of region that is characterized by spectral line emission from weakly ionized atoms. A prominent molecular ring is orbiting at a radius of 7–20 kly (2–6 kpc), which is providing a star-forming region of gas and dust. The nucleus appears decoupled and there is a counter-rotating element of stars and gas in the outer parts of the nucleus, suggesting a recent interaction with a smaller galaxy.

Scope: Planewave 12.5" CDK
Camera: Apogee U16M w Astrodon Generation II HaRGB Filter set
14x10 min Luminance
9 / 9 / 7 x 10 min RGB
Lucknow, Ontario, Canada
April - May 2023
Camera temp -25C
Images captured w TheSkyX and CCD-Commander
Processed in PixInsight with some processing in Photoshop CC 2023


- BlurX and NoiseX on the L and RGB masters
- Curves and HistogramTransformation on both masters
- SPCC colour calibration on the RGB master
- Saturation boost of the highlights in the RGB master
- Local Histogram Equalization (masked) on the L master (highlights only)


- layer the Luminance onto the RGB
- spot cleanup
- desaturation of the background (slight)