|Home  ||Galleries  ||Articles  ||Reviews  ||Best Gear  ||New  ||About  ||Contact  ||Gallery Index  ||Previous  ||
This galaxy in the Constellation Sculptor has a length almost the diameter of the full Moon. The galaxy is a wonderful sight in small telescopes when high in the sky with intricate dark lanes visible in larger amateur telescopes. The massive dust areas are locations where intense star formation is occurring and NGC 253 is called a starburst galaxy for this reason. The galaxy is about 11 million light years away.
This is a natural color image. The high dynamic range of astrophotos must be stretched to bring out the range of details the camera recorded. But the typical image stretch process loses color for brighter subjects (e.g. stars and the brighter parts of deep sky objects become whiter as they are made brighter). This image uses a new algorithm, rnc-color-stretch that does not lose color during the stretch. How do we know the colors are reasonable? The star colors can be checked against stellar photometry. Red stars have B-V > 2, orange stars have B-V of 1 to about 2. The blue-white stars have B-V in the range of 0 to -0.5. The colors closely follow the color sequence in Table 1 at Color of Stars. Solar-type stars have a B-V of 0.63 and appear close to white (daylight white balance).
Technical. Canon 7D Mark II 20-megapixel digital camera and 300 mm f/2.8 L IS II at f/2.8 plus a 1.4x teleconverter giving 420 mm at f/4, ISO 3200 and 2-arc-seconds per pixel. Fifty Eight 31-second exposures at ISO 3200 were added (30 minutes total exposure). I would normally use ISO 1600 and 60-second exposures, but seeing was bad, the object was only about 20 degrees off the horizon, and it was breezy, so I shortened the exposure in case of camera shake and to try and catch moments of stable atmosphere. I actually took 2 hours worth of data with the galaxy 22 degrees above the horizon at the start to only 18 degrees at the end of the imaging session. At that low altitude, atmospheric turbulence usually destroys resolution. But looking through the images, there are moments of exceptional stability for this altitude, enabling assembly of a pretty impressive result. Full resolution image is at 2.0 arc-seconds per pixel, and the image here is 1.5 arc-seconds per pixel, thus higher sampling than the camera resolution. No dark frame subtraction, no flat fields. Tracking with an astrotrac and no guiding.
Post processing: Converted in photoshop ACR, aligned with deep sky stacker using 2x drizzle, then stretched with rnc-color-stretch. Also see Astrophotography Image Processing Basic Work Flow. I applied Richardson-Lucy deconvolution to improve resolution on the stacked and stretched result.
The Exposure Factors, CEF, CEFA are measures of the relative amounts of light received from a subject. It can be used to fairly compare wildly different lens/telescope apertures and exposure times. For this image:
Modern DSLRs like the 7D Mark II include On-Sensor Dark Current Suppression Technology and low fixed pattern noise at ISOs around 1600 and higher, making no need for dark frame subtraction. Modern raw converters correct for light fall-off (flat field correction on linear sensor data) and also correct for hot/dead/stuck pixels. This makes processing low light images easy: simply align and average. See my series on Astrophotography Image Processing for more details.
To learn how to obtain stunning images like this, please visit my Extensive Articles on Photography .
See my review of the Canon 7D Mark II and why it is so good for astrophotography: Canon 7D Mark II sensor analysis.
Keywords to this image = astrophoto-1 galaxy Messier night low-light digital_astro canon_7d2
Image ID: ngc253.420mm.c11.18.2017.0J6A3408-510av58rs.h-0.66xc1-1500s.jpg
Obtaining Images or Prints
Last updated July 31, 2020