November 17, 2024

M82 – Spiral Galaxy in Ursa Major

M82 – Spiral Galaxy in Ursa Major

Telescope: Astro-Tech 8” f/8 Ritchey-Chretien, Orion Atlas EQ-G

Camera: ZWO ASI294MC Pro, 0C, Gain 200

Filter: 2” Orion Imaging Skyglow Filter

Guide scope: Astro-Tech 60mm, Meade DSI Pro II, PHD

Exposure: 57x240sec, saved as FITS

Darks: 32x240s, saved as FITS

Flats: 32×0.25sec, sky flats taken at dusk

Average Light Pollution: Red zone, Bortle 8, poor transparency, bright moonlight

Lensed Sky Quality Meter: 17.6 mag/arc-sec^2

Stacking: Mean with a 2-sigma clip.

White Balance: Nebulosity Automatic

Software: Nebulosity, Deep Sky Stacker, Photoshop

M82 is a close company to the nearby spiral galaxy M81 which is located about ½ degree to the south. These two form an interacting pair and M82 bears the scars of a close encounter with M82 about 100 million years ago. The dark dust lanes that cut across the central region of the galaxy are very distinctive and are easily visible in modest telescopes. M82 was originally classified as an irregular galaxy, but detailed studies had shown that it is actually a spiral seen nearly edge-on.

Copernicus – 11/28/2020, 21h30m EST

Telescope: Celestron C9.25 @ f/20, Orion Atlas EQ-G

Camera: ZWO ASI294MC, Gain 285

Filter: Highpoint Scientific IR Filter

Exposure: 64×0.01sec, saved as FITS

Seeing: fair, 3/5

White Balance: Nebulosity Automatic

Software: Sharpcap Pro, Nebulosity, Registax, Photoshop

Copernicus and its rays is one of the most beautiful structures on the lunar nearside and can even be seen with the naked eye as a bright region near the center of Oceanus Procellarum. The crater is 57 miles across, but only about 2.4 miles deep, making it about the same profile as a dinner plate. High resolution images of craterlets that radiate out from Copernicus reveal fishbone-like dunes that formed from the interference pattern of shockwaves that were generated during the formation of these crater chains some 800 million years ago. You can also see terraces circling the walls of Copernicus that formed as the terrain subsided after the impact. The smooth flat floor of the crater was selected as a landing site for one of the canceled Apollo 18-20 missions.  This image is one of a set taken as part of the first-light check-out of the new to me C9.25.

Fixing Mirror Flop

I just finished putting my new to me C9.25 back together. It had the classic symptom of not holding collimation and not holding focus after slewing. I suspect that this scope has never been taken apart as there were spots of fungus on the inside of the corrector and the corrector was really stuck! I marked its orientation, sprayed around the edge with Windex, and carefully worked it loose. I reached down inside and engaged a wooden dowel with one of the spanner holes in the lock ring a nudged it. Sure enough, it was completely loose. I could turn it about 1/2 rotation without any resistance. Just a tad more, and it was snug. While I had it open I removed a few tiny spots off of the primary and secondary with lens tissues .(I _hate_ touching the mirrors, but sometimes you get lucky) The secondary also have a bit of fungus, now clean.  I carefully cleaned the inside of the corrector with Windex followed by breath and lens tissues. Before closing the tube I inverted it and used a puffer bulb to blow the dust out, and then carefully lowered the corrector back in place. I didn’t like the original tiny spacers, so I cut ribbons of black construction paper and layered them evenly around the corrector until the gap was full (about 5 layers total all the way around). I remounted the rail, reinstalled the finder, touched up the paint, and now it’s ready for testing. I love reconditioning these old scopes!

So far I’m 3 for 3 finding loose lock rings. Tomorrow I’m going to open up a 12″ that’s showing the same symptom. Gotta do something while it’s cloudy.