Beta Ursae Majoris

Beta Ursae Majoris
β Ursae Majoris
Ursa major star name.png
Merak in Ursa Major.
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ursa Major
Right ascension 11h 01m 50.5s
Declination +56° 22′ 57″
Apparent magnitude (V) +2.34
Characteristics
Spectral type A1V
U−B color index 0.01
B−V color index -0.02
Variable type suspected
Astrometry
Radial velocity (Rv) -12 km/s
Proper motion (μ) RA: 81.66 mas/yr
Dec.: 33.74 mas/yr
Parallax (π) 41.07 ± 0.60 mas
Distance 79 ± 1 ly
(24.3 ± 0.4 pc)
Absolute magnitude (MV) 0.41
Details
Mass 3 M
Radius 2 R
Luminosity 69 L
Temperature 9800 K
Metallicity ?
Rotation ~39 km/s.
Age ? years
Other designations
Merak, Merakh, 48 Ursae Majoris, HR 4295, HD 95418, BD+57 1302, FK5 416, HIP 53910, SAO 27876, GC 15145

Coordinates: Sky map 11h 01m 50.5s, +56° 22′ 57″ Beta Ursae Majoris (β UMa, β Ursae Majoris) is a star in the constellation of Ursa Major. It has the traditional name Merak.

It is more familiar to northern hemisphere observers as one of the "pointer stars" in the Big Dipper, and a straight line connecting it with nearby Alpha Ursae Majoris (Dubhe) extends to Polaris, the north star. It is also one of the five stars in the Big Dipper asterism that form a part of a loose open cluster called the Ursa Major moving group, sharing the same region of space and not just the same patch of sky by our perspective.

Merak is fairly typical for a main sequence star of its type, although being slightly hotter and larger than our own Sun, it shines several times brighter. It is surrounded by a cooling disk of dust, much like those discovered around Fomalhaut and Vega. No planets have been discovered orbiting Merak, but the presence of the dust indicates they may exist or be in the process of forming.

The name is derived from the Arabic المراق al-maraqq "the loins" (of the bear).

Book plate by Sydney Hall depicting Ursa Major's stars

Merak in Military

USS Merak (1918) and USS Merak (AF-21), both of United States navy ship.


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