Cor Caroli

Cor Caroli · Double star · CVn

Visible as soon as it's properly dark (22:15); highest around 20:22, 40° up in the WNW. Easy naked-eye target, unmistakable even from a light-polluted yard. The pair splits cleanly at moderate power.

Magnitude
2.9
Angular size
Surface brightness
Altitude now
22°
Azimuth now
303° WNW
Moon separation
69°
Rise
05:16
Transit
20:22 (40°)
Set
02:16
Best window
20:22–22:34 CEST
Tonight score
86 · Excellent tonight

Easy wide pair.

Tonight's sky

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

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.

Splitting this pair: Resolvable

Separation 19.3″ against a Dawes limit of 0.58″ for 200 mm. Components magnitude 2.9 and 5.5, position angle 229°.

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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