56 Ursae Majoris

Star in the constellation Ursa Major From Wikipedia, the free encyclopedia

56 Ursae Majoris (56 UMa) is a binary star in the constellation Ursa Major. At an apparent magnitude of 5.03, it is a faint star but visible to the naked eye depending on factors such as light pollution and eyesight. Parallax measurements derive a distance of 555 light-years.

Quick facts Constellation, Right ascension ...
56 Ursae Majoris
Observation data
Epoch J2000      Equinox ICRS
Constellation Ursa Major
Right ascension 11h 22m 49.58373s[1]
Declination +43° 28 57.7267[1]
Apparent magnitude (V) 5.03[2]
Characteristics
Spectral type G7IIIBa0.3[3]
U−B color index +0.82[4]
B−V color index +1.02[4]
Astrometry
Radial velocity (Rv)1.01±0.05[5] km/s
Proper motion (μ) RA: −35.561 mas/yr[6]
Dec.: −10.651 mas/yr[6]
Parallax (π)5.8813±0.0930 mas[6]
Distance555 ± 9 ly
(170 ± 3 pc)
Orbit[7]
Period (P)16,911+438
−401
days
Semi-major axis (a)22.9+1.0
−1.1
AU
Eccentricity (e)0.562+0.012
−0.012
Inclination (i)68+3.6
−3.4
°
Longitude of the node (Ω)60+3
−3
°
Periastron epoch (T)2468401+432
−385
Argument of periastron (ω)
(secondary)
286+2.3
−2.3
°
Details[7]
56 UMa A
Mass4.3±0.2 M
Radius21.16±0.86[8] R
Surface gravity (log g)2.30[8] cgs
Temperature4,917±34[8] K
Metallicity [Fe/H]0.05 dex
56 UMa B
Mass1.31+0.11
−0.12
 M
Other designations
BD+44°2083, FK5 2908, HD 98839, HIP 55560, HR 4392, SAO 43719
Database references
SIMBADdata
Close

It is a single-lined spectroscopic binary with an orbital period of about 45 years.[5] The primary is an evolved giant star with a spectral class G7IIIBa0.3, a Barium star.[3] The companion star is likely a heavy neutron star born by a supernova that exploded around 100,000 years ago.[7]

References

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