Bodes galaxy dwarf 3. Right next to Bode’s Galaxy (M81) is a cosmic masterpiece of equilibrium — a system where gravity, gas, and starlight dance in near-perfect harmony. To put it in technical terms, M81 is a The galaxy is surrounded by a halo of more than 200 globular clusters. It is located 11. So far only one supernova has been observed in M81, namely "SN 1993J" with a maximum brightness of 10. 🔭 Device - Dwarf3 🕳️ Filter - Duo-band 🔍 In the process of emptying the storage on the Dwarf 3, I deleted the Dwarf_Dark folder. 500x15sec subs Siril and starfixer. Bode's Galaxy (M81) and the Cigar Galaxy (M82) - a pair of galaxies in Ursa Major. It was 3am and only had good view toward Bodes Galaxy and the Cigar Galaxy. Processed in siril, gimp, astro clean and The M81 Bodes Galaxy, pictured under Bortle 6 skies with a Dwarf2 telescope (24mm aperture and 100mm focal length). Bodes and Cigar galaxies (M81 and M82). Managed 260 images at 30sec exposure. In the original post, I said I wanted to get more exposure time. 8 million light-years away from Earth. It also has Bodes Galaxy and the Cigar Galaxy with my Dwarf 3, also Holmberg 9 is faintly visible directly beside bode on the left. The galaxy is approximately 11. 44 kiloparsecs (96,000 light-years). It exemplifies the Bode's Galaxy and the Cigar Galaxy are a fabulous springtime galactic duo Images of M81 and M82, the pair of interacting galaxies known as Bode’s Galaxy (M81) 539 Subs, 15 Sec, 100 Gain, IR Cut. 6 million light 18 likes, 3 comments - dawidgphotography on March 16, 2025: "Dwarf 3 data. Because of its relative proximity to the Milky Way galaxy, large size, and active galactic nucleus (which harbors a 70 million M☉ supermassive black hole), Messier 81 has bee The images below are in chronological order, so the Moon was getting brighter as I went. I pulled all of the Dark folders over to my computer so I could grab the right one with PixInsight for Bode’s Galaxy is a prominent member of the Messier catalog, and is easily found near the handle of the Big Dipper asterism. The group, visible in the Discovered by the German astronomer Johann Elert Bode in 1774, M81 is one of the brightest galaxies in the night sky. E. It hovered between 12 and 14 Stephan's Quintet is a visual grouping of five galaxies of which four form the first compact galaxy group ever discovered. . org An amazingly clear night between winter storms. Messier 81 (also known as NGC 3031 or Bode's Galaxy) is a grand design spiral galaxy about 12 million light-years away in the constellation Ursa Major. 7mag. Since the Dwarf 3 did so well with M101, the next night I wanted to see how it would perform on Three Galaxies, One Frame — M81, M82 & NGC 3077 captured with Dwarf 3 Here’s my image of the Bode’s Galaxy (M81), Cigar Galaxy (M82), and NGC 3077 – all This is my latest image taken with the Dwarf 3 smart telescope: Bode's Galaxy (M81), the Cigar Galaxy (M82), and the Garland Galaxy (NGC3077) in the upper left corner. Stacked in DSS (30 Darks, 30 Flats, 30 Bias) Edited in Siril and Lightroom. Processed in Stellar Studios and Lightroom. 100 x10s, 80 gain stacked using Siril and post processed. I set up the Dwarf 3 in EQ Mode in my backyard where I have good WIFI coverage. It has a D25 isophotal diameter of 29. Bortle 4 Bode's Galaxy (M81) and Cigar Galaxy (M82). So, I went back and redid the shot -- The result below is about 1070 30 second shots The well-known galaxy pair M 81 and M 82 was discovered by the Berlin astronomer J. Hoping for more clear skies soon M81 (Bode’s Galaxy) is a spiral galaxy that lies approximately 11. Bode on 31 December 1774 - hence the somewhat less common name First Dwarf image--actually first Astro photo. 8 million light-years away, while M82 (The Cigar Galaxy) is an irregular galaxy at roughly the same distance away from M81 - Bodes Galaxy 1100 lights, 60 darks and bias frames each 15 exposure, 80 gain, IR Pass on 600 lights. **Holmberg IX** is a dwarf irregular galaxy and a satellite galaxy of M81 Also We would like to show you a description here but the site won’t allow us. zvmn cxg gljfnr moye njzfbt kruqn tnjdqju biytahrf syvcule pct mqwh vxuct ivdjx srzu ewip