Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ursa Major |
Right ascension | 13h 40m 44.27335s [2] |
Declination | +54° 40′ 53.8891″ [2] |
Apparent magnitude (V) | 4.69 - 4.75 [3] |
Characteristics | |
Spectral type | M2 III [4] |
B−V color index | +1.630±0.006 [5] |
Variable type | SRb [3] |
Astrometry | |
Radial velocity (Rv) | −18.61±0.20 [6] km/s |
Proper motion (μ) |
RA: −19.06
[2]
mas/
yr Dec.: −10.56 [2] mas/ yr |
Parallax (π) | 6.23 ± 0.22 mas [2] |
Distance | 520 ± 20
ly (161 ± 6 pc) |
Absolute magnitude (MV) | −1.39 [5] |
Details | |
Mass | 1.1 [7] M☉ |
Radius | 80 [8] R☉ |
Luminosity | 1,250 [9] L☉ |
Surface gravity (log g) | 0.62 [7] cgs |
Temperature | 3,579 [7] K |
Metallicity [Fe/H] | −0.07 [7] dex |
Other designations | |
Database references | |
SIMBAD | data |
83 Ursae Majoris is a candidate binary star [11] system in the northern circumpolar constellation of Ursa Major. It is a semiregular variable star, and it has been given the variable star designation IQ Ursae Majoris. It ranges in brightness from apparent visual magnitude 4.69 to 4.75. [3] Percy and Au (1994) identified it as a small amplitude red variable with an irregular behavior, having a characteristic time scale of 20 days. [12] Based upon an annual parallax shift of 6.23±0.22 mas, [2] it is located roughly 520 light years from the Sun. The distance derived from its Gaia Early Data Release 3 parallax is 179 pc. [13] The system is moving closer with a heliocentric radial velocity of −18.6 [6] km/s.
The visible component is an evolved red giant with a stellar classification of M2 III. [4] It is a marginal barium star, showing an enhanced abundance of s-process elements in its outer atmosphere. This material may have been acquired during a previous mass transfer from a now white dwarf companion, or self-enriched by a dredge-up during the asymptotic giant branch process. [14]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ursa Major |
Right ascension | 13h 40m 44.27335s [2] |
Declination | +54° 40′ 53.8891″ [2] |
Apparent magnitude (V) | 4.69 - 4.75 [3] |
Characteristics | |
Spectral type | M2 III [4] |
B−V color index | +1.630±0.006 [5] |
Variable type | SRb [3] |
Astrometry | |
Radial velocity (Rv) | −18.61±0.20 [6] km/s |
Proper motion (μ) |
RA: −19.06
[2]
mas/
yr Dec.: −10.56 [2] mas/ yr |
Parallax (π) | 6.23 ± 0.22 mas [2] |
Distance | 520 ± 20
ly (161 ± 6 pc) |
Absolute magnitude (MV) | −1.39 [5] |
Details | |
Mass | 1.1 [7] M☉ |
Radius | 80 [8] R☉ |
Luminosity | 1,250 [9] L☉ |
Surface gravity (log g) | 0.62 [7] cgs |
Temperature | 3,579 [7] K |
Metallicity [Fe/H] | −0.07 [7] dex |
Other designations | |
Database references | |
SIMBAD | data |
83 Ursae Majoris is a candidate binary star [11] system in the northern circumpolar constellation of Ursa Major. It is a semiregular variable star, and it has been given the variable star designation IQ Ursae Majoris. It ranges in brightness from apparent visual magnitude 4.69 to 4.75. [3] Percy and Au (1994) identified it as a small amplitude red variable with an irregular behavior, having a characteristic time scale of 20 days. [12] Based upon an annual parallax shift of 6.23±0.22 mas, [2] it is located roughly 520 light years from the Sun. The distance derived from its Gaia Early Data Release 3 parallax is 179 pc. [13] The system is moving closer with a heliocentric radial velocity of −18.6 [6] km/s.
The visible component is an evolved red giant with a stellar classification of M2 III. [4] It is a marginal barium star, showing an enhanced abundance of s-process elements in its outer atmosphere. This material may have been acquired during a previous mass transfer from a now white dwarf companion, or self-enriched by a dredge-up during the asymptotic giant branch process. [14]