Menu

IC 405

4-8 inch Telescope • Emission Nebulae Detailed

IC 405 (C31)

Image: Nielander

IC 405 finder map.

Finder map for IC 405

The popular name “Flaming Star Nebula” is derived from its appearance in long-exposure color astrophotography. It is a well-known and frequently imaged target among amateur astrophotographers. Best observed when high in the sky to reduce atmospheric extinction and improve contrast, particularly from mid-northern latitudes. Its very low surface brightness makes IC 405 highly susceptible to light pollution. In 4–8 inch telescopes, the nebula appears as a faint, uneven glow around the central star, while the dramatic contrast between red emission and blue reflection regions seen in images is not visually detectable.

IC 405 finder optic view.

Finder scope & binocular view of IC 405

PropertyValue
Common namesFlaming Star Nebula, Caldwell 31
Catalog namesC 31, IC 405, SH 2-229, vdB 34, LBN 795, …
TypeInterstellar Medium
SubtypeHII Region
Coordinates5h 17m 24.00s, +34° 22’ 60.00”
SeasonNovember - January
Best monthMid-December
Beginner friendlyNo
Visual rewardLow
Filters requiredUHC, H-beta
LP toleranceLow
Minimum equipmentSmall telescope
Optimal equipmentMedium telescope
Magnitude6.0
Size30.0 arcminutes x 20.0 arcminutes
ConstellationAuriga

Observation Notes

Naked Eye

Not visible to the naked eye, though the bright star AE Aurigae is obvious.

Binoculars

Generally not visible. Under exceptional dark-sky conditions, very experienced observers using large binoculars may suspect a vague brightening around AE Aurigae, but reliable detection is uncommon.

Small Telescope

Under very dark, transparent skies, a small telescope with an H-beta filter may reveal an extremely faint, uneven glow surrounding AE Aurigae. The nebula is subtle and easily missed; without a filter it is typically invisible.

Medium Telescope

In an 8–10 inch telescope from a dark site, an H-beta filter provides the best chance of detection. The nebula appears as a very faint, ghostly haze, with the main curved arc being the most likely feature to glimpse using averted vision. Even then, the view is low contrast and uncertain.

Large Telescope

A 12-inch or larger telescope improves detection but does not transform the object. The nebula remains diffuse and delicate, with only hints of uneven brightness and curvature visible. Any impression of structure is subtle, and the nebula’s large extent is appreciated more by context than by sharply defined features.

Observing IC 405 from your latitude

From mid-northern latitudes (~40°N), IC 405 reaches a maximum altitude of about 84° above the southern horizon and stays above the horizon for about 16h 49m, best placed December - February.

Your latitudeMax altitudeHours above horizon
60°N (≈ Oslo, Helsinki, Anchorage)64°Circumpolar (24h)
50°N (≈ London, Prague, Vancouver)74°19h 32m
40°N (≈ Madrid, New York, Beijing)84°16h 49m
30°N (≈ Cairo, Houston, Delhi)86°15h 13m
20°N (≈ Honolulu, Mexico City, Mumbai)76°14h 1m
10°N (≈ Chennai, Bangalore, Bangkok)66°13h 1m
(≈ Quito, Nairobi, Singapore)56°12h 5m
20°S (≈ Rio de Janeiro, Antananarivo, Alice Springs)36°10h 11m
35°S (≈ Sydney, Cape Town, Buenos Aires)21°8h 19m
45°S (≈ Christchurch, Hobart, Puerto Montt)11°6h 25m

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, IC 405 rises at 02:16 AM, is highest in the sky at 10:43 AM (84° above the horizon), and sets at 07:10 PM.

Altitude
Azimuth
Max Altitude
83.7°
Rises
02:16 AM
Sets
07:10 PM
Transit
10:43 AM
IC 405: RA 5h 17m 24.00s, Dec +34° 22' 60.00"
Computed for the night of July 13–14, 2026 (New York).