Little Dumbbell

M76 · Planetary nebula · Per

Circumpolar from here — up all night, best placed around 04:28, due N. 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
10.1
Angular size
3.0′
Surface brightness
21.1 mag/arcsec²
Altitude now
35°
Azimuth now
49° NE
Moon separation
69°
Rise
Transit
04:28 (87°)
Set
Best window
20:22–07:10 CEST
Tonight score
60 · Not realistic with 200 mm at Bortle 8

Tonight's sky

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

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

A UHC filter lifts contrast noticeably here; an OIII is even stronger on planetary nebulae, at the cost of some star field.

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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