M29

M29 · Open cluster · Cyg

Circumpolar from here — up all night, best placed around 23:10, due S. At the edge of visibility from this sky — needs a dark-adapted eye, averted vision and low power for maximum contrast.

Magnitude
7.1
Angular size
7.0′
Surface brightness
20.0 mag/arcsec²
Altitude now
76°
Azimuth now
135° SE
Moon separation
116°
Rise
Transit
23:10 (80°)
Set
Best window
20:22–06:04 CEST
Tonight score
71 · Good

Tonight's sky

0°15°30°45°60°75°90°21:0022:0023:0000:0001:0002:0003:0004:0005:0006:0007:00min 20°now
  • M29

Through your instrument

40× · TFOV 1.70° · exit pupil 5.00 mm · f/6.0

The eye's colour receptors need far more photons than a camera sensor collects over minutes, so faint deep-sky objects genuinely look grey at the eyepiece.

200 mm f/6 Dobsonian at 40×

Newtonian: image rotated 180°

Ad slot · object-simulator · 300 × 250

Your optics, in numbers

Aperture
200 mm
Focal ratio
f/6.0
Magnification
40×
True field
1.70°
Exit pupil
5.00 mm
Dawes limit
0.58″
Rayleigh limit
0.69″
Max useful power
250×
Limiting magnitude
11.6

Recommended settings

Low power: 30 mm (40×, exit pupil 5.0 mm)

A 5–7 mm exit pupil gives the darkest sky background per unit of object brightness — best for large faint nebulae and star clouds.

High power: 6 mm (200×)

Planets, the Moon and double stars take up to about 2× the aperture in mm, capped at your 250× seeing limit.

Aperture verdict

200 mm is well matched to this target.

Filters

Nebula filters do not help — galaxies and clusters emit across the spectrum. Darker skies do.

Technique

Dark-adapt for 20–30 minutes, use averted vision on faint targets, tap the tube gently to catch motion, and wait for the object to reach transit rather than shooting over rooftops.

Seeing vs transparency

Planets need steady air (seeing); faint deep-sky objects need clean, transparent air. A hazy but still night is a planet night.

Gear for this object

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