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Alpha Persei

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Also 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°
View on SIMBAD →

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
Sources (3)

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.

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