‹ Night of 3 October 2026

The Orion Nebula, wide

The Orion Nebula, wide

Messier 42 and Messier 43

Five overlapping fields joined into one, to take in the faint outer loops of gas round the bright heart of the nebula.

What you are looking at

The Orion Nebula, wide, with its parts named, a scale bar and north marked

Swipe sideways to see the rest. Tap the picture for full size.

Distance
1,344 light-years
This picture spans
27 light-years
The light left
Around the year 680
What it is
The nearest great nursery of new stars

For photographers

A 2 x 2 mosaic round the deep centre field; each outline is one sensor frame, with frames kept of frames taken.

The Orion Nebula, wide, with the frames that were joined outlined

Swipe sideways to see the rest. Tap the picture for full size.

Exposures
20 s at ISO 3200 throughout; 2 s at ISO 800 for the core
Frames
Centre 39 of 69. Panels 13, 12, 5 and 2 of 13 each: the last two were shot under cloud and are shown in grey
Mosaic
Each panel centred by plate solve, then placed by its own plate solution; scaled on shared stars; matched to the centre with a constant and a plane; feathered
Sampling
1.552 arcsec per pixel (2 x 2 mean of the working grid). Stars 4.4 to 5 arcsec wide
Field
67.9 x 43.4 arcmin, cropped level from the mosaic; one frame is 38.8 x 25.9
When
4 October 2026, before dawn. 41 to 46 degrees up, Moon up, thin cloud passing
Calibration
Flat from 26 twilight-sky frames, large-scale shape from cloud-lit frames. No darks
Stacking
RAW colour planes (no demosaic), hot pixels by 3 x 3 median, registered on stars with rotation, sigma-clipped mean
Finish
Black 34 and white 199 of 255, S-curve 0.3. Saturation x 1.5. Dark sky made neutral and smoothed (bilateral, 3 px)
Telescope
Celestron 8SE Schmidt-Cassegrain with dew shield: 203 mm aperture, 2,084 mm focal length (measured by plate solve), f/10.3
Camera
Sony a6000, stock, at prime focus: APS-C 23.5 x 15.6 mm, 6000 x 4000, 3.9 micron pixels, RAW
Mount
Sky-Watcher EQ6-R, unguided. Set down 27 degrees off the pole; both axes driven from a pointing model fitted to plate solves. Residual drift about 0.1 arcsec per second

© 2026 Brad Gessler · Celestron 8SE (8 inch, 2,080 mm) and Sony a6000 on an EQ6-R · San Francisco Bay Area · 4 October 2026
Capture and mount: Observatory (Elixir on a Raspberry Pi 3). Stacking: numpy, OpenCV, rawpy. Plate solving: astrometry.net. Stacked from the camera's RAW frames. Nothing generated.

© 2026 Brad Gessler. The pictures and the words are his own; all rights reserved.