HIP 57274

HIP 57274 is a star in the northern circumpolar constellation of Ursa Major with a system of three planets. It is invisible to the naked eye, having an apparent visual magnitude of 8.96. The distance to this system is 84.4 light years based on stellar parallax, and it is drifting further away with a radial velocity of +30 km/s. The star has a relatively high rate of proper motion, traversing the celestial sphere at the rate of 0.382 arcsecond/year.

HIP 57274
Observation data
Epoch J2000      Equinox J2000
Constellation Ursa Major
Right ascension 11h 44m 40.9643s
Declination +30° 57 33.4509
Apparent magnitude (V) 8.96
Characteristics
Spectral type K5 V
U−B color index +1.06
B−V color index +1.111±0.016
Astrometry
Radial velocity (Rv)+29.76±0.35 km/s
Proper motion (μ) RA: −27.069±0.081 mas/yr
Dec.: −381.708±0.079 mas/yr
Parallax (π)38.6381 ± 0.0499 mas
Distance84.4 ± 0.1 ly
(25.88 ± 0.03 pc)
Absolute magnitude (MV)6.89
Details
Mass0.73±0.05 M
Radius0.68±0.03 R
Luminosity0.19±0.01 L
Surface gravity (log g)4.71±0.1 cgs
Temperature4,640±100 K
Metallicity [Fe/H]+0.09±0.05 dex
Rotation45 d
Rotational velocity (v sin i)0.5±0.5 km/s
Age7.87±5 Gyr
Other designations
BD+31° 2290, Gaia DR2 4021079911593673600, GJ 439, HIP 57274, SAO 62684, LTT 13227, 2MASS J11444095+3057339
Database references
SIMBADdata
ARICNSdata

This is an ordinary K-type main-sequence star with a stellar classification of K5V. It appears to be older than the Sun with an age of roughly eight billion years and is spinning slowly with a projected rotational velocity of under 1 km/s. The star has 73% of the mass of the Sun and 68% of the Sun's radius. The abundance of elements heavier than helium is about the same or slightly higher than in the Sun. The star is radiating just 19% of the luminosity of the Sun from its photosphere at an effective temperature of 4,640 K.

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