Double binary star system in the constellation Ursa Major
Iota Ursae Majoris
Location of ι Ursae Majoris (circled) |
Observation data Epoch J2000 Equinox J2000
|
Constellation
|
Ursa Major
|
Right ascension
|
08h 59m 12.45362s[1]
|
Declination
|
+48° 02′ 30.5741″[1]
|
Apparent magnitude (V)
|
3.14[2]/10.1/10.3
|
Characteristics
|
Spectral type
|
A7V(n)[3] + M3V + M4V[4]
|
U−B color index
|
+0.08[2]
|
B−V color index
|
+0.19[2]
|
Variable type
|
Suspected
|
Astrometry |
---|
|
---|
Radial velocity (Rv) | +9.0[5] km/s |
Proper motion (μ) | RA: -441.29[1] mas/yr Dec.: -215.32[1] mas/yr |
Parallax (π) | 68.92 ± 0.16 mas[1] |
Distance | 47.3 ± 0.1 ly (14.51 ± 0.03 pc) |
Absolute magnitude (MV) | +2.31[6] |
|
Orbit[7] |
---|
Primary | ι UMa A |
Companion | ι UMa BC |
Period (P) | 2084 ± 15 yr |
Semi-major axis (a) | 16.7 ± 0.3″ |
Eccentricity (e) | 0.90 ± 0.02 |
Inclination (i) | 54 ± 4° |
Longitude of the node (Ω) | 134 ± 2° |
Periastron epoch (T) | B 2029 ± 1 |
Argument of periastron (ω) (secondary) | 23 ± 5° |
Details |
---|
ι UMa Aa |
---|
Mass | 1.7 ± 0.1[4] M☉ |
Radius | 1.67[8] R☉ |
Luminosity | 8.98[8] L☉ |
Surface gravity (log g) | 4.30 ± 0.07[4] cgs |
Temperature | 8,242[9] K |
Metallicity [Fe/H] | 0.01±0.05[8] dex |
Rotational velocity (v sin i) | 154[10] km/s |
Age | 620[11] Myr |
Bb |
---|
Mass | 1±0.3[4][12] M☉ |
|
---|
ι UMa B |
---|
Mass | 0.35 ± 0.05[4] M☉ |
Radius | 0.46[13] R☉ |
ι UMa C |
---|
Mass | 0.30 ± 0.05[4] M☉ |
Radius | 0.43[13] R☉ |
Other designations |
---|
Talitha, ι Ursae Majoris, ι UMa, Iota UMa, 9 Ursae Majoris, BD+48 1707, FK5 335, GJ 331, HD 76644, HIP 44127, HR 3569, SAO 42630, WDS J08592+4803A,BC. [3] |
Database references |
---|
SIMBAD | ι UMa |
| ι UMa A |
| ι UMa BC |
ARICNS | ι UMa A |
| ι UMa B |
| ι UMa C |
Iota Ursae Majoris (ι Ursae Majoris, abbreviated Iota UMa, ι UMa), also named Talitha ,[14] is a star system in the northern circumpolar constellation of Ursa Major. It has an apparent visual magnitude of 3.14,[2] making it visible to the naked eye and placing it among the brighter members of this constellation. Based upon parallax measurements, it is located at a distance of 47.3 light-years (14.5 parsecs) from the Sun.
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- ^ "Sixth Catalog of Orbits of Visual Binary Stars". United States Naval Observatory. Archived from the original on 1 August 2017. Retrieved 16 May 2017.
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- ^ "IAU Catalog of Star Names". Retrieved 28 July 2016.