HD 115404
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Coma Berenices |
| HD 115404 A | |
| Right ascension | 13h 16m 51.051430s |
| Declination | +17° 01′ 01.840901″ |
| Apparent magnitude (V) | 6.66 |
| HD 115404 B | |
| Right ascension | 13h 16m 51.554014s |
| Declination | +17° 00′ 59.892133″ |
| Apparent magnitude (V) | 9.50 |
| Characteristics | |
| U−B color index | +0.64 |
| B−V color index | +0.92 |
| HD 115404 A | |
| Spectral type | K2 V |
| HD 115404 B | |
| Spectral type | M0.5 V |
| Astrometry | |
| HD 115404 A | |
| Radial velocity (Rv) | 7.62 ± 0.09 km/s |
| Proper motion (μ) | RA: 636.285±0.028 mas/yr Dec.: −264.678±0.031 mas/yr |
| Parallax (π) | 91.0176±0.0236 mas |
| Distance | 35.834 ± 0.009 ly (10.987 ± 0.003 pc) |
| HD 115404 B | |
| Radial velocity (Rv) | 5.95±0.13 km/s |
| Proper motion (μ) | RA: 649.666±0.031 mas/yr Dec.: −263.937±0.026 mas/yr |
| Parallax (π) | 90.9475 ± 0.0232 mas |
| Distance | 35.862 ± 0.009 ly (10.995 ± 0.003 pc) |
| Orbit | |
| Period (P) | 770.0 yr |
| Semi-major axis (a) | 8.06″ |
| Eccentricity (e) | 0.12 |
| Inclination (i) | 93.41° |
| Longitude of the node (Ω) | 104.66° |
| Periastron epoch (T) | B 1875.0 |
| Argument of periastron (ω) (secondary) | 276.99° |
| Details | |
| HD 115404 A | |
| Mass | 0.70 ± 0.09 M☉ |
| Radius | 0.76 ± 0.02 R☉ |
| Luminosity | 3.1 L☉ |
| Surface gravity (log g) | 4.58 ± 0.03 cgs |
| Temperature | 4976 K |
| Metallicity [Fe/H] | −0.08 dex |
| Rotational velocity (v sin i) | 2.8 km/s |
| Age | 10.2 (5.4–13.5) Gyr |
| HD 115404 B | |
| Mass | 0.542 M☉ |
| Radius | 0.550 R☉ |
| Other designations | |
| BD+17° 2611, GJ 505, HD 115404, HIP 64797, SAO 100491, LHS 2713 | |
| Database references | |
| SIMBAD | A |
| B | |
| ARICNS | A |
| B | |
HD 115404 is a binary star system located in the constellation Coma Berenices. Parallax measurements made by Hipparcos put the system at 36 light-years, or 11 parsecs, away. The combined apparent magnitude of the system is 6.52, with the magnitudes of the components being 6.66 and 9.50.
The primary component, designated A, is a K-type main sequence star. It is about 70% as massive as the Sun, and is 0.76 times as wide. Its companion is a red dwarf (M0.5 V). It has 54.2% the mass of the Sun, and is 0.55 times as wide. The two stars orbit each other every 770 years, and are separated by about 8″. The system is thought to be fairly old, at 5.4 to 13.5 billion years old.
In 2022, two exoplanets, Neptunian and super-Jovian in mass, were discovered in orbit around the primary star using a combination of radial velocity and astrometry.
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥0.097+0.020 −0.022 MJ |
0.088+0.003 −0.004 |
10.5+0.001 −0.002 |
0.232+0.197 −0.138 |
— | — |
| c | 10.319+1.473 −1.209 MJ |
11.364+3.301 −1.905 |
15319.2+7240.3 −3526.2 |
0.211+0.173 −0.102 |
25.791+1.842 −2.157° |
— |