‹ Night of 3 October 2026

The Pleiades

The Pleiades

Messier 45, the Seven Sisters

A family of about a thousand young stars, born together some 100 million years ago. The blue haze round Merope and Maia is a dust cloud they are drifting through, lit by their light.

What you are looking at

The Pleiades, with its parts named, a scale bar and north marked

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

Distance
444 light-years
This picture spans
13 light-years
The light left
In 1582, the year the modern calendar began
Honest note
The glow round Atlas and Pleione is thin cloud that night, not nebula

For photographers

A 3 x 3 mosaic; each outline is one sensor frame, with frames kept of frames taken.

The Pleiades, with the frames that were joined outlined

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

Exposures
10 s at ISO 1600, about 7 frames per panel: one minute each
Frames
72 taken, 60 kept: 10 minutes in all. Panels 3 and 7 were shot through cloud and only fill where clear panels have no data
Mosaic
Each panel centred to 0.6 arcmin by plate solve and a local nudge. Placed by its own plate solution (shared stars agree to 0.5 arcsec); one brightness scale and one constant per panel; feathered
Sampling
1.553 arcsec per pixel. Stars about 5 arcsec wide; the bright ones are saturated and left white
Field
99 x 63 arcmin, cropped level from the mosaic; one frame is 38.8 x 25.8
When
4 October 2026, before dawn, over 49 minutes. 74 degrees up, 41 percent Moon in the sky
What is real
The haze at Merope and Maia repeats between independent stacks at 4 to 11 sigma. The glow at Atlas and Pleione is cloud
Calibration
Flat and dust map from tonight's clouded frames; a faint sensor pattern common to all panels removed. No darks
Finish
Black 24 of 255, gamma 0.95. Saturation x 1.45. Dark sky made neutral and smoothed (median 5 px, then bilateral 5 px): faint haze traded for a quiet sky
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.