Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Hydra |
Right ascension | 09h 56m 57.83878s[1] |
Declination | −15° 53′ 42.4291″[1] |
Apparent magnitude (V) | 7.41[2] |
Characteristics | |
Spectral type | F7V[3] |
Apparent magnitude (B) | 7.920[2] |
Apparent magnitude (J) | 6.505±0.019[2] |
Apparent magnitude (H) | 6.344±0.038[2] |
Apparent magnitude (K) | 6.224±0.023[2] |
B−V color index | 0.510±0.011[2] |
Astrometry | |
Radial velocity (Rv) | 7.39±0.13[1] km/s |
Proper motion (μ) | RA: −14.313±0.024 mas/yr[1] Dec.: −65.057±0.024 mas/yr[1] |
Parallax (π) | 14.8646 ± 0.0214 mas[1] |
Distance | 219.4 ± 0.3 ly (67.27 ± 0.10 pc) |
Absolute magnitude (MV) | 3.23[2] |
Details | |
Mass | 1.46±0.01 M☉[4] 1.36+0.04 −0.05 M☉[5] 1.42[6] M☉ |
Radius | 1.53±0.02 R☉[4] 1.88[6] R☉ |
Luminosity | 4.02±0.04[4] L☉ |
Surface gravity (log g) | 4.13±0.04[5] cgs |
Temperature | 6,616±39[4] K |
Metallicity [Fe/H] | 0.26±0.03 Dex[7] +0.202[6] dex |
Rotational velocity (v sin i) | 12.8±0.5[6] km/s |
Age | 0.8±0.2 Gyr[4] 2.78+0.47 −0.70 Gyr[5] 2.24[6] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
HD 86264 is a single[9] star with an exoplanetary companion in the equatorial constellation of Hydra. It is too faint to be readily visible to the naked eye with an apparent visual magnitude of 7.41.[2] The distance to this star, as determined by parallax measurements, is 219 light-years, and it is drifting further away with a radial velocity of +7.4 km/s.[1] A 2015 survey ruled out the existence of any stellar companions at projected distances above 30 astronomical units.[9]
This is an F-type main-sequence star with a stellar classification of F7V.[3] It is about two billion years old with a modest level of chromospheric activity and is spinning with a projected rotational velocity of 13 km/s.[6] The star is larger and more massive compared to the Sun, and it has a higher metallicity – the abundance of elements with a higher atomic number than helium.[6] It is radiating four times the luminosity of the Sun from its photosphere at an effective temperature of 6,616 K.[4]
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