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Andromeda

COSMOS / CONSTELLATIONS / AND

Andromeda

IAU abbreviation And. One of the 48 classical constellations listed by Ptolemy in the Almagest in the 2nd century AD.

STAR CHART

MirachAlpheratzAlmachδ AndNembusο And↑ N ← E
Coloured dots are the stars of Andromeda brighter than magnitude 6.5 (size by brightness, colour by temperature); grey dots are stars brighter than 5.5 in neighbouring constellations. North is up, east to the left. Constellation boundaries and traditional stick figures are not drawn.

KEY FACTS

IAU abbreviation
And
Latin name / genitive
Andromeda / Andromedae
Position
Right ascension ≈ 0 h 43 m; declination +23° to +53°
Visibility from Türkiye
Visible in full from anywhere in Türkiye. When it crosses the meridian its centre stands about 88° above the horizon from Ankara.
Best time to observe
Best placed at 21:00 Türkiye time around 28 November.
Number of stars
158 stars brighter than magnitude 6.5 in the catalogue; 30 brighter than 5 and 8 brighter than 4.

INTERACTIVE LAB

Where is Andromeda tonight?

The lab opens for Ankara on today’s date. Drag the time slider through the night; the “Best night” button jumps to the date when the constellation is highest at 21:00 (around 28 November). Change the city to compare the view from elsewhere in Türkiye and around the world.

MYTH, HISTORY AND OBSERVING

In Greek myth Andromeda is the Ethiopian princess chained to a rock as an offering to a sea monster and rescued by Perseus. Its best-known object is the Andromeda Galaxy (M31), about 2.5 million light-years away and visible to the naked eye as a faint smudge under dark skies. The star Alpheratz marks the north-eastern corner of the Great Square of Pegasus.

BRIGHTEST STARS

StarMagnitudeDistance (light-years)Spectral type
Alpheratz2.0797B9p
Mirach2.07197M0IIIvar
Almach2.10393B8V
δ And3.27106K3III
Nembus3.59177K3III
ο And3.62687B6pv
λ And3.8186G8III-IV
μ And3.86130A5V

Magnitude: apparent brightness; the smaller the number, the brighter the star. Distances derive from parallax measurements and are uncertain for distant stars. Source: HYG v4.1 star catalogue (CC BY-SA 4.0).

SOURCES

Position, visibility and best observing time were computed approximately for this page from the catalogue stars (Ankara, 39.9° N). The 88 constellations were adopted by the IAU in 1922; their boundaries were drawn by Eugène Delporte in 1930.

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