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Beta Monocerotis

4-8 inch Telescope • Challenging Doubles Beta Monocerotis finder map.

Finder map for Beta Monocerotis

While lacking ancient mythological significance, Beta Monocerotis is celebrated in amateur astronomy as one of the finest showpiece multiple stars, sometimes informally referred to as the “Wonder Star” because of its telescopic beauty. Best observed near culmination, when it is highest in the sky and atmospheric seeing is typically most favorable for resolving the close components. Resolving the tight B–C component pair (about 2.8 arcseconds separation) requires steady atmospheric conditions (good seeing) and typically a 4-inch (100 mm) or larger telescope

Beta Monocerotis finder optic view.

Finder scope & binocular view of Beta Monocerotis

PropertyValue
Common namesThe Wonder Star
Catalog names-
TypeStar
SubtypeDouble Star
Coordinates6h 28m 49.07s, -7° 01’ 59.01”
SeasonDecember - February
Best monthJanuary
Beginner friendlyYes
Visual rewardHigh
Filters requiredNone
LP toleranceHigh
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude3.7
Size-
ConstellationMonoceros

Observation Notes

Naked Eye

Appears as a single, moderately bright star in Monoceros, in the general winter Milky Way region east of Orion.

Binoculars

Remains unresolved as a single point of light. Any perceived color is subtle and not a primary feature at this scale.

Small Telescope

Under good seeing, a small telescope (around 3–4 inches) at moderate to high magnification can resolve the brighter A and B components as a close but distinct pair. The split is seeing-dependent and not guaranteed every night.

Medium Telescope

A 5–8 inch telescope reliably resolves all three components. The fainter C component becomes clearly visible, and the stars form a graceful, gently curved arrangement that makes this system a classic showpiece double.

Large Telescope

Provides a clean, comfortable separation of all three stars at a range of magnifications. The system appears crisp and well balanced, though the visual appeal lies in the geometry and separation rather than strong color contrast.

Observing Beta Monocerotis from your latitude

From mid-northern latitudes (~40°N), Beta Monocerotis reaches a maximum altitude of about 43° above the southern horizon and stays above the horizon for about 11h 18m, best placed December - February.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)23°10h 31m
50°N (≈ London, Prague, Vancouver)33°11h
40°N (≈ Madrid, New York, Beijing)43°11h 18m
30°N (≈ Cairo, Houston, Delhi)53°11h 33m
20°N (≈ Honolulu, Mexico City, Mumbai)63°11h 44m
10°N (≈ Chennai, Bangalore, Bangkok)73°11h 55m
(≈ Quito, Nairobi, Singapore)83°12h 5m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)77°12h 25m
35°S (≈ Sydney, Cape Town, Buenos Aires)62°12h 45m
45°S (≈ Christchurch, Hobart, Puerto Montt)52°13h 3m

Altitudes and durations are geometric, computed for each latitude, independent of date. Set your location below for tonight's exact rise, transit, and set times.

Visibility from New York

From New York tonight, Beta Monocerotis rises at 06:16 AM, is highest in the sky at 11:54 AM (42° above the horizon), and sets at 05:32 PM.

Altitude
Azimuth
Max Altitude
42.3°
Rises
06:16 AM
Sets
05:32 PM
Transit
11:54 AM
Beta Monocerotis: RA 6h 28m 49.07s, Dec -7° 01' 59.01"
Computed for the night of July 13–14, 2026 (New York).