Alpha Persei
Sign in to saveAlso known as Mirfak, 33 Persei, * alf Per
star in the constellation Perseus
Astronomical data · SIMBAD
- Object type
- V*
- Spectral type
- F5Ib
- Distance
- 506 light-years
- Redshift
- z = -0.0000071982872668074904
- Coordinates
- RA 51.0807° · Dec 49.8612°
via SIMBAD · CDS Strasbourg
Key facts
- Constellation
- Perseus
- Right ascension
- 03 24 19.37009
- Declination
- +49 ° 51 ′ 40.2455 ″
- Spectral type
- F5 Ib
- U b color index
- +0.38
- B v color index
- +0.483
via Wikipedia infobox
Wikidata facts
- Distance from Earth
- 156
- Radius
- 55.0
- Mass
- 7.3
- Image
- Alpha Persei Cluster.png
Show 16 more facts
- spectral class
- F3I
- catalog code
- UBV M 40922
- stellar rotational velocity
- 18
- apparent magnitude
- 0.54
- right ascension
- 51.08070871833
- declination
- 49.86117929306
- effective temperature
- 6350
- parallax
- 6.44
- radial velocity
- -2.158
- surface gravity
- 20.4
- metallicity
- 7.3
- luminosity
- 5000
- absolute magnitude
- -5.1
- right ascension component of proper motion
- 25
- declination component of proper motion
- -24
- age estimated by a dating method
- 0.041
via Wikidata · CC0
~5 min read
Article
Alpha Persei (Latinized from α Persei, abbreviated Alpha Per, α Per), formally named Mirfak (pronounced /ˈmɜːrfæk/ or /ˈmɪərfæk/), is the brightest star in the northern constellation of Perseus, outshining the constellation's best-known star, Algol (β Persei). Alpha Persei has an apparent visual magnitude of 1.8, and is a circumpolar star when viewed from mid-northern latitudes.
Alpha Persei lies in the midst of a cluster of stars named as the eponymous Alpha Persei Cluster, or Melotte 20, which is easily visible in binoculars and includes many of the fainter stars in the constellation. Determined distance using the trigonometric parallax, places the star 510 light-years (160 parsecs) away.