HD 115404

HD 115404
Observation data
Epoch J2000      Equinox J2000
Constellation Coma Berenices
HD 115404 A
Right ascension 13h 16m 51.05143s
Declination +17° 01′ 01.8409″
Apparent magnitude (V) 6.66
HD 115404 B
Right ascension 13h 16m 51.55401s
Declination +17° 00′ 59.8921″
Apparent magnitude (V) 9.50
Characteristics
HD 115404 A
Evolutionary stage main sequence
Spectral type K2 V
U−B color index +0.623
B−V color index +0.917
HD 115404 B
Evolutionary stage main sequence
Spectral type M0.5 V
B−V color index +1.232
Astrometry
HD 115404 A
Radial velocity (Rv)7.62 ± 0.09 km/s
Proper motion (μ) RA: 636.285(28) mas/yr
Dec.: −264.678(31) mas/yr
Parallax (π)91.0176±0.0236 mas
Distance35.834 ± 0.009 ly
(10.987 ± 0.003 pc)
Absolute magnitude (MV)+6.3
HD 115404 B
Radial velocity (Rv)5.95±0.13 km/s
Proper motion (μ) RA: 649.666(31) mas/yr
Dec.: −263.937(26) mas/yr
Parallax (π)90.9475±0.0232 mas
Distance35.862 ± 0.009 ly
(10.995 ± 0.003 pc)
Absolute magnitude (MV)10.1
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
Mass0.70±0.09 M
Radius0.76±0.02 R
Luminosity3.1 L
Surface gravity (log g)4.58±0.03 cgs
Temperature4976 K
Metallicity [Fe/H]−0.08 dex
Rotation18.2 days
Rotational velocity (v sin i)2.8 km/s
Age10.2 (5.4–13.5) Gyr
HD 115404 B
Mass0.542 M
Radius0.550 R
Luminosity0.043 L
Surface gravity (log g)4.90 cgs
Temperature3,709 K
Rotational velocity (v sin i)9.6 km/s
Age3.0 Gyr
Other designations
BD+17°2611, GJ 505, HD 115404, HIP 64797, SAO 100491, LHS 2713
Database references
SIMBADA
B
Exoplanet Archivedata
ARICNSA
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 reported in orbit around the primary star using a combination of radial velocity and astrometry. However, a 2025 study using radial velocity observations failed to detect these planets.

The HD 115404 A planetary system
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b (disputed) ≥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 (disputed) 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
°