Astrophotography diagnosis of N?buleuse du Requin sombre: Sensor tilt and satellite trail
Raw60s23 juin 2026
The Doc examined this image of N?buleuse du Requin sombre (raw, 60s). Estimated overall technical quality: 5/10. 2 defects found: Sensor tilt (severity 4/5), Satellite trail (severity 1/5).
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Info
- Cible
- N?buleuse du Requin sombre
- Date
- 23 juin 2026, 23:38
- Lune
- Croissant décroissant 30% (6.8° d'alt., 115.2° de la cible)
- Site
- Bortle 1 · ciel pristine (VIIRS)
- Position
- 22h11m06s · +73°09'38"
Very favorable conditions. Bortle 1 is the best possible context for a dark nebula like the Shark, a target that lives only on faint reflected light and contrast against the background: every magnitude of sky darkness translates directly into nebulosity detection. The Moon at 30% illumination, only 6.8 deg above the horizon and 115 deg from the target, contributes almost no light pollution: its flux is largely absorbed by the atmospheric path at that altitude and its angular distance is comfortable. The stated 2.5 arcsec seeing remains the real limiting factor, consistent with the 4.7 px FWHM (about 6.7 arcsec) measured at center, which mostly reflects the optical defect rather than the atmosphere.
Setup
- Type d'image
- Brut
- Télescope
- C11+Hyper+Uranus
- Caméra
- Poseidon-C PRO
- Exposition
- 60s
- Phase de lune
- Gibbeuse croissante (65 %)
- Seeing
- 2.5
- FOV
- 2.48°
Powerful but demanding setup. A C11 in Hyperstar configuration at 540mm f/1.9 with a 6252x4176 sensor yields 2.48 deg of field, which frames the Shark Nebula, a wide diffuse object, nicely. The 1.436 arcsec/px sampling suits 2.5 arcsec seeing well, neither over nor undersampled. The downside is that f/1.9 imposes backfocus and flatness tolerances of a few tens of microns: the measured tilt is a direct consequence of that demand, not of a gross error. On settings, gain 125 and offset 50 are healthy, no dark clipping, sensor at -10C is fine. The background-to-black-point margin of 2 is low, but at f/1.9 under Bortle 1 with 60s that is expected: the sky is simply very dark.
The diagnosis in detail
The diagnosis comes down to one structuring point: focal plane flatness. The Moffat measurements trace a sharp gradient from edge to edge, 1.3 px FWHM upper right against 8.3 px lower right, with an intermediate and nearly round center. Field curvature or incorrect backfocus would degrade all four corners symmetrically; here a single axis tips over, and the vertical asymmetry (0.219 against 0.036 horizontal) confirms the signature. The major-axis orientations follow the tip as well, from PA -28 deg upper left to PA 60 deg lower right.
The center at elong 1.12, just above the debayer floor, shows tracking is sound over 60s: no drift or guiding oscillation would spare the center and hit a single corner. The problem is purely mechanical, in the optical train.
At f/1.9 the depth of focus is on the order of ten microns: a sensor tipped by a few hundredths of a degree is enough to produce exactly this map. Until that adjustment is made, there is no point collecting hours: stacking will average already-smeared stars and no processing will recover them. The rest of the frame is healthy, with a clean sky background and consistent exposure.
Priority actions
- Correct sensor tilt with a push-pull tilt ring, iterating on test frames measured with the Aberration Inspector
- Aim for under 15% FWHM spread between corners before launching a long series
- Re-check backfocus after tilt correction, since tolerance at f/1.9 is a few tens of microns
- Check the tightness and concentricity of every adapter in the Hyperstar train
- Plan at least 10 to 15 subs so sigma rejection removes the satellite trail





