Pleiades

M45 · Open cluster · Tau

Best around 06:34, high in the S. Too low-surface-brightness to see from Bortle 8 with 200 mm f/6 Dobsonian — this needs a darker sky, not more aperture or magnification.

Magnitude
1.6
Angular size
1.8°
Surface brightness
20.4 mag/arcsec²
Altitude now
-0°
Azimuth now
50° NE
Moon separation
50°
Rise
22:28
Transit
06:34 (65°)
Set
Best window
00:52–07:10 CEST
Tonight score
74 · Good
Pleiades photographed
Image: NASA, ESA, AURA/Caltech

Tonight's sky

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

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×

Object larger than field of view — use a lower-power eyepiece.

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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