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11 Ursae Minoris
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11 Ursae Minoris
11 Ursae Minoris
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Ursa Minor
Right ascension 15h 17m 05.88946s[1]
Declination +71° 49′ 26.0473″[1]
Apparent magnitude (V) 5.15[2]
Characteristics
Spectral type K4 III[3]
Apparent magnitude (B) 6.664[2]
Apparent magnitude (J) 2.657[2]
Apparent magnitude (H) 1.931±0.192[2]
Apparent magnitude (K) 1.701±0.198[2]
B−V color index 1.514±0.004[2]
Astrometry
Radial velocity (Rv)−17.80±0.12[1] km/s
Proper motion (μ) RA: +4.073 mas/yr[1]
Dec.: +9.477 mas/yr[1]
Parallax (π)7.9260±0.1249 mas[1]
Distance412 ± 6 ly
(126 ± 2 pc)
Absolute magnitude (MV)–0.37[4]
Details
Mass2.60+0.48
−0.44
[5] M
Radius29.14±0.45[5] R
Luminosity250±6[6] L
Habitable zone inner limit15.63±0.57[5] AU
Habitable zone outer limit30.65±1.10[5] AU
Surface gravity (log g)1.78±0.04[6] cgs
Temperature4,253±25[6] K
Metallicity−0.02±0.05[6]
Age639+507
−278
[5] Myr
Other designations
11 UMi, BD+72°678, FK5 1140, HD 136726, HIP 74793, HR 5714, SAO 8207, PPM 8870, GCRV 8864[7]
Database references
SIMBADdata
Exoplanet Archivedata

11 Ursae Minoris is a single[8] star located approximately 410 light years away[1] in the northern circumpolar constellation of Ursa Minor. The star is visible to the naked eye as a faint, orange-hued star with an apparent visual magnitude of 5.15.[2] It is moving closer to the Earth with a heliocentric radial velocity of −17.8 km/s.[1]

This is an aging K-type giant star with a stellar classification of K4 III.[3] It is 600 million years old with twice the mass of the Sun. As a consequence of exhausting the hydrogen at its core, the star has expanded to 29 times the Sun's radius.[5] It is radiating 250 times the luminosity of the Sun from its swollen photosphere at an effective temperature of 4,253 K.[6]

11 Ursae Minoris is sometimes named Pherkard or Pherkad Minor, the later name to distinguish it from Pherkad (Major) which is γ Ursae Minoris. It has also been designated as γ1 Ursae Minoris, in which case the brighter Pherkad is called γ2 Ursae Minoris, but these names are rarely used.[9] 11 Ursae Minoris is the Flamsteed designation.

11 Ursae Minoris has a detected planet discovered in August 2009.[4]

Planetary system

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11 Ursae Minoris b was discovered during a radial velocity survey of 62 K type Red giant stars using the 2m Alfred Jensch telescope of the Thuringian State Observatory in Germany.[4]

A newer mass measurement of the host star implies a larger planetary mass of 14.15±1.23 MJ, which would make 11 Ursae Minoris b a low-mass brown dwarf.[5]

The 11 Ursae Minoris planetary system[4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b ≥14.15±1.23 MJ 1.54 ± 0.07 516.22 ± 3.25 0.08 ± 0.03

References

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