Blue supergiant · Perseus
Menkib
Also known as: ξ Persei (ξ Per), HIP 18614
mag 4.01,200 light-years
About
Menkib (ξ Persei) is a blue supergiant of magnitude 4.0 in Perseus, about 1,200 light-years away.
How to find it
- Menkib is in the constellation Perseus.
- Best evenings: around early January it is highest at about 9 pm (10 pm in summer time); a month earlier, two hours later.
- Where on Earth: it is seen well, at least 10° up, from north of 44° S.
When it rises and sets tonight, how high it climbs and how much the Moon gets in the way are worked out in your browser for your place.
What you will see
- EyesVisible from the suburbs on a clear night, but lost in bright city skies.
- Binoculars (10×50)A sharp point; binoculars bring out its colour and the fainter stars around it.
- Telescope (6–8 inch)Still a point of light at any magnification — stars are too far away to show a disc. Low in the sky, bright stars twinkle and flash colours.
Stars look the same in any instrument: brighter and sharper, but never bigger.
Facts
| Proper name | Menkib |
|---|---|
| Designation | ξ Persei (ξ Per) |
| Hipparcos number | HIP 18614 |
| Type | Blue supergiant |
| Spectral type | O7.5Iab: |
| Colour | WhiteB−V colour index 0.02 |
| Magnitude | 4.0The smaller the number, the brighter. |
| Distance | 1,200 light-yearsThe light you see left it around AD 800. Distances this large are uncertain by 10% or more. |
| Proper motion | 0.003″ per year across the sky |
| Constellation | Perseus |
| Right ascension (J2000) | 03h 58m 57.9s |
| Declination (J2000) | +35° 47′ 28″ |
More in Perseus
NGC 869Double ClusterOpen cluster · mag 3.7
M34Spiral ClusterOpen cluster · mag 5.2
M76Little Dumbbell NebulaPlanetary nebula · mag 11.5
NGC 1275Perseus AGalaxy · mag 12.2
Mel 20Alpha Persei ClusterOpen cluster · mag 1.2
NGC 1499California NebulaEmission nebula · mag 5.0
NGC 1545m & m Double ClusterOpen cluster · mag 6.2
NGC 1528m & m Double ClusterOpen cluster · mag 6.4Sources and credits
Star data: HYG Database by David Nash, CC BY-SA 4.0. All data sources →