Asterism Atlas

Named star-patterns beyond the official constellation boundaries.

Ursa Major

Big Dipper

Plough, Charles's Wain

common observer pattern · high confidence

The famous ladle is the brightest northern guide-pattern: use Merak-to-Dubhe to hop to Polaris, then follow the bent handle to Arcturus. At 50°N it is circumpolar but rides highest on spring evenings.

Central RA
12h 20m 02.0s
Central Dec
+55° 34′ 47″
Brightest member
V 1.77
Best months from 50°N
March–June evenings
Suggested instrument
naked-eye
Approx. span
25.7°
Megrez / 69Del UMa (HR 4660) — V 3.31Phecda / 64Gam UMa (HR 4554) — V 2.44Merak / 48Bet UMa (HR 4295) — V 2.37Mizar / 79Zet UMa (HR 5054) — V 2.27Alkaid / 85Eta UMa (HR 5191) — V 1.86Dubhe / 50Alp UMa (HR 4301) — V 1.79Alioth / 77Eps UMa (HR 4905) — V 1.77AliothDubheAlkaidMizarMerakPhecdaMegrezbrighter → largerV 1 reference1V 3 reference3V 5 reference5
Ursa Major 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: 25.7°; use at least 36.0° field for context.

Observing and imaging

Naked eye

Primary naked-eye pattern; suburban skies should show the main stars unless the description notes a low horizon or dark-sky need.

Binoculars

Binoculars are optional: use them to check colours, nearby doubles, or richer Milky Way background.

Small scope

A telescope is usually too narrow for the whole shape; use it after the pattern has guided you to a target.

Imaging

Frame as a wide-field scene in/near Ursa Major; a field of view around 36° 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: 7/7 stars — fully visibleBortle 5: 7/7 stars — fully visibleBortle 7: 7/7 stars — fully visible

Member stars

NameBayer / FlamsteedHRRA J2000Dec J2000V mag
Alioth77Eps UMaHR 490512h 54m 01.7s+55° 57′ 35″1.77
Dubhe50Alp UMaHR 430111h 03m 43.7s+61° 45′ 03″1.79
Alkaid85Eta UMaHR 519113h 47m 32.4s+49° 18′ 48″1.86
Mizar79Zet UMaHR 505413h 23m 55.5s+54° 55′ 31″2.27
Merak48Bet UMaHR 429511h 01m 50.5s+56° 22′ 57″2.37
Phecda64Gam UMaHR 455411h 53m 49.8s+53° 41′ 41″2.44
Megrez69Del UMaHR 466012h 15m 25.6s+57° 01′ 57″3.31

Source and confidence

common observer pattern; high confidence. Commonly used constellation-part or seasonal guide-pattern name, with member-star positions plotted from BSC5.

Citations