HD 125595

HD 125595 is a star with a close Neptunian companion in the southern constellation of Centaurus. With an apparent visual magnitude of 9.03, this star is too faint to be viewed with the naked eye. It is located at a distance of 92 light years from the Sun based on parallax measurements, and is drifting further away with a radial velocity of +4.5 km/s. The star has a high proper motion, traversing the celestial sphere and an angular rate of 0.57 arcsecond yr−1.

HD 125595
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Centaurus
Right ascension 14h 21m 23.186s
Declination −40° 23 38.22
Apparent magnitude (V) 9.03
Characteristics
Evolutionary stage Main sequence
Spectral type K4V(k)
Apparent magnitude (B) 10.137
Apparent magnitude (J) 7.097±0.021
Apparent magnitude (H) 6.608±0.026
Apparent magnitude (K) 6.447±0.023
B−V color index 1.107±0.006
Astrometry
Radial velocity (Rv)+4.48±0.45 km/s
Proper motion (μ) RA: −561.636 mas/yr
Dec.: −68.516 mas/yr
Parallax (π)35.4337 ± 0.0762 mas
Distance92.0 ± 0.2 ly
(28.22 ± 0.06 pc)
Absolute magnitude (MV)6.80
Details
Mass0.77 M
Radius0.73+0.02
−0.03
 R
Luminosity0.241 L
Surface gravity (log g)4.58 cgs
Temperature4,672 K
Metallicity [Fe/H]0.13 dex
Rotation37.2±2.0 d
Rotational velocity (v sin i)1.50 km/s
Age8.17 Gyr
Other designations
CD−39°8857, GJ 545.1, HD 125595, HIP 70170, PPM 319432, LHS 2900, LPM 523, LTT 5648, NLTT 37029, GCRV 64739
Database references
SIMBADdata
Exoplanet Archivedata

This is an ordinary K-type main-sequence star with a stellar classification of K4V(k), which indicates it is a small star that is generating energy at its core through hydrogen fusion. It is about eight billion years old and is spinning with a projected rotational velocity of 1.5 km/s, giving it a 37 day rotation period. The star shows a moderate level of chromospherically activity due to star spots or plagues. It is smaller, cooler, dimmer, and less massive than the Sun, but shows a higher atmospheric metallicity.

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