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NGC 3718
NGC660
Twisted Spiral Galaxy in Ursa Major

Click here for higher-resolution versions: 65% Cropped(1899x1899) 100% Cropped; (2921x2921) 50% uncropped (2030x2030)

 

NGC 3718NGC 3718 is the twisted spiral galaxy in the lower part of the image. Its odd shape likely is the result of gravitational interactions with the smaller spiral galaxy, NGC 3729, above it. Immediately to the left of NGC 3718 is the Hickson Compact Group 56 (HCG 56), which consists of five interacting galaxies. NGC 3718 is thought to be about 52 million light years from us; at that distance, it has a diameter of about 35,000 light years (about a third that of our Milky Way galaxy). HCG 56 is thought to be about 425 million light years away.

As usual, there are a lot of background galaxies in this photo.

The entire field of the photo is about the same width as a full moon.

 

Technical Information:

LRGB: 570:180:195:240 (a total of almost 20 hours of exposures); luminance layer consists of a blend of 34 fifteen-minute images and 20 three-minute images, all using a luminance filter; R channel is 12 fifteen-minute images taken through a red filter; G consists of 13 fifteen-minute images taken through a green filter, while B is the combination of 12 twenty-minute images taken through a blue filter. I gathered a lot of Ha data, but it added nothing, so ended up not using it.

Equipment: RC Optical Systems 14.5 inch Ritchey-Chrétien carbon fiber truss telescope, with ion-milled optics and RCOS field flattener, at about f/9, and an SBIG STX-16803 with internal filter wheel (SBIG filter set), guided by an SBIG AO-X/STX Guider, all riding on a Bisque Paramount ME German Equatorial Mount.

Image Acquisition/Camera Control: Maxim DL, controlled with ACP Expert/Scheduler, working in concert with TheSky X.

Processing: All images calibrated (darks, bias and sky flats), aligned, and combined in Pixinsight. Color combine in Pixinsight. Some finish work (background neutralization, color calibration, Noise XTerminator and Blur XTerminator, gradient removal) done in Pixinsight; some finish work (LRGB combination, contrast and saturation adjustment) was done in Photoshop CC.

Location: Data acquired remotely from Sierra Remote Observatories, Auberry, California, USA.

Date: Images taken on many nights from December 2023 through March 2024. Image posted September 26, 2024.

Date: Image scale of full-resolution image: 0.56 arcseconds per pixel.

Seeing: Generally good

CCD Chip temperature: -25C

Copyright 2023, 2024 Mark de Regt

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