HD 125595
Observation data Epoch J2000.0 Equinox J2000.0 |
|
---|---|
Constellation | Centaurus |
Right ascension | 14h 21m 23.186s[1] |
Declination | −40° 23′ 38.21″[1] |
Apparent magnitude (V) | 9.03 |
Characteristics | |
Spectral type | K4V |
Apparent magnitude (B) | 10.13 |
Apparent magnitude (J) | 7.097 |
Apparent magnitude (H) | 6.608 |
Apparent magnitude (K) | 6.447 |
B−V color index | 1.10 |
Astrometry | |
Radial velocity (Rv) | 3.1 km/s |
Proper motion (μ) | RA: −561.46 ± 1.05[1] mas/yr Dec.: −67.06 ± 0.85[1] mas/yr |
Parallax (π) | 35.77 ± 1.04[1] mas |
Distance | 91 ± 3 ly (28.0 ± 0.8 pc) |
Absolute magnitude (MV) | 6.84 |
Details | |
Mass | 0.68 M☉ |
Radius | 0.78 ± 0.07 R☉ |
Luminosity | 0.239 ± 0.020 L☉ |
Surface gravity (log g) | 4.29 cgs |
Temperature | 4590 ± 100 K |
Metallicity | 0.02 |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Extrasolar Planets Encyclopaedia |
data |
HD 125595 is a 9th magnitude K-type main sequence star located approximately 89 light years away in the constellation Centaurus. This star is smaller, cooler, dimmer, and less massive than our Sun. Also its metal content is 4% more than the Sun. In 2009, a gas giant planet was found in orbit around the star.
Planetary system
HD 125595 b is an extrasolar planet which orbits the star. This planet has at least 14 times the mass of Earth and takes 9 days and 16 hours to orbit the star at a semimajor axis of 0.081 AU.[2]
Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
---|---|---|---|---|---|---|
b | ≥0.045 MJ | 0.0809 ± 0.0014 | 9.6737 ± 0.0039 | 0 | — | — |
See also
References
Coordinates: 14h 21m 23.1859s, −40° 23′ 38.211″
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