Asterism Atlas

Named star-patterns beyond the official constellation boundaries.

Vulpecula

Coathanger

Brocchi's Cluster, Collinder 399

modern informal / binocular asterism · high confidence

Brocchi's Cluster is the binocular asterism that really looks like its name: a straight bar with a dangling hook. It is easy to sweep up between Altair and Albireo.

Central RA
19h 46m 56.3s
Central Dec
+22° 36′ 17″
Brightest member
V 4.58
Best months from 50°N
June–September evenings
Suggested instrument
7x50
Approx. span
11.4°
7 Vul (HR 7409) — V 6.3314 Vul (HR 7641) — V 5.675 Vul (HR 7390) — V 5.6316 Vul (HR 7657) — V 5.224 Vul (HR 7385) — V 5.1617 Vul (HR 7688) — V 5.079 Vul (HR 7437) — V 5.0012 Vul (HR 7565) — V 4.9515 Vul (HR 7653) — V 4.6413 Vul (HR 7592) — V 4.5813 Vul15 Vul12 Vul9 Vul17 Vul4 Vul16 Vulbrighter → largerV 1 reference1V 3 reference3V 5 reference5
Vulpecula contextschematic finder — bright-star context, not a constellation boundary mapNE

Finder context

This wider chart is deliberately schematic: it uses nearby bright-star context and boxes the asterism’s member-star footprint, but it does not draw official constellation boundaries or promise horizon/season precision.

Framing: Approximate member-star span: 11.4°; use at least 15.9° field for context.

Observing and imaging

Naked eye

Possible as a haze or partial pattern only from darker skies; use naked-eye stars nearby for the hop.

Binoculars

Best treated as a binocular field; start with 7×50 or similar and allow roughly 11.4° of pattern spread.

Small scope

Use low power only; higher magnification breaks the pattern into separate stars.

Imaging

Frame as a wide-field scene in/near Vulpecula; a field of view around 16° keeps context without claiming exact constellation boundaries.

Observability from your latitude

Uses this asterism’s centroid RA/Dec: transit altitude, hours above 20°, and a month-scale evening window. Default is Edmonton-ish 50°N.

Naked-eye visibility by sky class

Approximate limiting magnitudes: Bortle 3 ≈ V 6.6, Bortle 5 ≈ V 5.6, Bortle 7 ≈ V 4.6. The shape is counted recognisable when at least 70% of defining stars clear the limit.

Bortle 3: 10/10 stars — fully visibleBortle 5: 7/10 stars — partialBortle 7: 1/10 stars — washed out

Member stars

NameBayer / FlamsteedHRRA J2000Dec J2000V mag
13 Vul13 VulHR 759219h 53m 27.7s+24° 04′ 47″4.58
15 Vul15 VulHR 765320h 01m 06.1s+27° 45′ 13″4.64
12 Vul12 VulHR 756519h 51m 04.1s+22° 36′ 36″4.95
9 Vul9 VulHR 743719h 34m 34.9s+19° 46′ 24″5.00
17 Vul17 VulHR 768820h 06m 53.4s+23° 36′ 52″5.07
4 Vul4 VulHR 738519h 25m 28.6s+19° 47′ 55″5.16
16 Vul16 VulHR 765720h 02m 01.4s+24° 56′ 17″5.22
5 Vul5 VulHR 739019h 26m 13.2s+20° 05′ 52″5.63
14 Vul14 VulHR 764119h 59m 10.5s+23° 06′ 05″5.67
7 Vul7 VulHR 740919h 29m 20.9s+20° 16′ 47″6.33

Source and confidence

modern informal / binocular asterism; high confidence. Well-known binocular asterism name; the star pattern is informal even where associated with Brocchi’s Cluster / Collinder 399.

Citations