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Mu Cephei

Naked Eye • Variable Stars Mu Cephei finder map.

Finder map for Mu Cephei

Its ‘Garnet Star’ moniker is one of the most famous and evocative stellar nicknames in amateur astronomy, frequently used to introduce newcomers to the concept of stellar colors. Best viewed from the Northern Hemisphere, where it is circumpolar for many observers. It is inaccessible from most of the Southern Hemisphere. Perceiving its deep red color fully without proper dark adaptation; tracking its slow, subtle brightness variations over many months.

Mu Cephei finder optic view.

Finder scope & binocular view of Mu Cephei

PropertyValue
Common namesHerschel’s Garnet Star, Erakis
Catalog names-
TypeClassical Cepheid
SubtypeClassical Cepheid
Coordinates21h 43m 30.46s, +58° 46’ 48.17”
SeasonJuly - September
Best monthMid-August
Beginner friendlyMarginal
Visual rewardHigh
Filters requiredNone
LP toleranceHigh
Minimum equipmentNaked eye
Optimal equipmentNaked eye
Magnitude4.1
Size-
ConstellationCepheus

Observation Notes

Naked Eye

Visible from moderately dark skies as a noticeably orange-red star in Cepheus. Its brightness varies slowly and by a modest amount, with changes best appreciated over many months rather than from night to night.

Binoculars

The star’s warm orange-red coloration is more apparent, though the intensity of the color varies with sky conditions and contrast. The surrounding field provides useful comparison stars for long-term brightness estimates.

Small Telescope

Shows the star as a bright, unresolved point with a strong orange-red to reddish hue. The color is its principal visual feature; no disk or surface detail is visible.

Medium Telescope

Offers little additional visual information beyond enhancing the stability of the view for careful magnitude estimates. The perceived color may appear slightly deeper, but this effect is subjective.

Large Telescope

Provides no meaningful visual advantage for observing the star itself, which remains unresolved. Herschel’s Garnet Star is best appreciated for its color and slow variability rather than for telescopic detail.