Pi2 Ursae Minoris

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Pi2 Ursae Minoris
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Minor
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.89[2] (7.32 + 8.15)[3]
Characteristics
Spectral type F1V[4] + G0[5]
B−V Template:Engvar Template:Val[2]
Astrometry
Radial velocity (Rv)Template:Val[6] km/s
Proper motion (μ) RA: −32.643[1] mas/yr
Dec.: 41.425[1] mas/yr
Parallax (π)8.1090±0.2844 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)Template:Val[6]
Orbit[5]
Period (P)Template:Val yr
Semi-major axis (a)Template:Val
Eccentricity (e)Template:Val
Inclination (i)Template:Val°
Longitude of the node (Ω)Template:Val°
Periastron epoch (T)Template:Val
Argument of periastron (ω)
(secondary)
Template:Val°
Details
Mass1.87[7] Template:Solar mass
RadiusTemplate:Val[1] Template:Solar radius
LuminosityTemplate:Val[1] Template:Solar luminosity
TemperatureTemplate:Val[7] K
Metallicity [Fe/H]+0.09[7] dex
Age1.20[7] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[8]
Database references
SIMBADdata

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Pi2 Ursae Minoris, which is Latinized from π2 UMi / π2 Ursae Minoris, is a binary star system in the northern circumpolar constellation of Ursa Minor. The pair have a combined apparent visual magnitude of 6.89,[2] which can be viewed with a pair of binoculars.[9] They are located at a distance of approximately 400 light years from the Sun based on parallax, but are drifting closer with a radial velocity of −32 km/s.[6]

This star was found to be a double system by O. Struve in 1832, and the pair have now completed a full orbit. There is a lot of scatter in the data though,[5] so the grade of the orbital elements is rated as poor.[3] The system has a high eccentricity of 0.96 and they orbit each other with a period of roughly 172 years.[5] The magnitude 7.32 primary is an F-type main-sequence star with a stellar classification of F1V.[4] The fainter secondary has a magnitude of 8.15[3] and is G-type star.[5] At present the angular separation between both stars is 0.67 arcseconds [1].

References

Template:Reflist

Template:Stars of Ursa Minor

  1. a b c d e f g Cite error: Invalid <ref> tag; no text was provided for refs named GaiaDR2
  2. a b c Cite error: Invalid <ref> tag; no text was provided for refs named Anderson_Francis_2012
  3. a b c Cite error: Invalid <ref> tag; no text was provided for refs named Malkov_et_al_2012
  4. a b Cite error: Invalid <ref> tag; no text was provided for refs named ginestet_et_al_1999
  5. a b c d e Cite error: Invalid <ref> tag; no text was provided for refs named Hartkopf_et_al_2008
  6. a b c Cite error: Invalid <ref> tag; no text was provided for refs named Holmberg_et_al_2007
  7. a b c d Cite error: Invalid <ref> tag; no text was provided for refs named Casagrande_et_al_2011
  8. Cite error: Invalid <ref> tag; no text was provided for refs named SIMBAD
  9. Cite error: Invalid <ref> tag; no text was provided for refs named ICQ