Observation data EpochJ2000 EquinoxJ2000 | |
---|---|
Constellation | Cetus |
Right ascension | 00h 15m 28.11090s[1] |
Declination | −16° 08′ 01.6303″[1] |
Apparent magnitude (V) | 11.483[2] |
Characteristics | |
Spectral type | M3.5V[3] |
Astrometry | |
Radial velocity (Rv) | -26.43 ± 0.1[4] km/s |
Proper motion (μ) | RA: 731.83[1]mas/yr Dec.: -607.73[1]mas/yr |
Parallax (π) | 166.6±0.3 mas[3] |
Distance | 19.58 ± 0.04 ly (6.00 ± 0.01 pc) |
Absolute magnitude (MV) | 12.70 ± 0.01 / 15.12 ± 0.09[3] |
Orbit[3] | |
Period (P) | 4.55726+0.00075 −0.00074y.[5] |
Semi-major axis (a) | 0.3037 ± 0.0005″ |
Eccentricity (e) | 0.36136+0.00097 −0.00098[5] |
Inclination (i) | 143.93+0.25 −0.24[5]° |
Longitude of the node (Ω) | 62.8 ± 0.4° |
Periastronepoch (T) | JD 2449850.4 ± 0.8 |
Argument of periastron (ω) (secondary) | 166.6 ± 0.5° |
Details[3] | |
GJ 1005 A | |
Mass | 0.179 ± 0.002 M☉ |
Temperature | 3341±224[6] K |
Metallicity [Fe/H] | -0.41[5] dex |
GJ 1005 B | |
Mass | 0.112 ± 0.001 M☉ |
Other designations | |
Gaia DR2 2368293487260807040,HIP 1242,G 158-50,G 266-76,LHS 1047,LP 764-87,LTT 114,2MASS J00152799-1608008 | |
Database references | |
SIMBAD | data |
ARICNS | A |
B | |
Location of GJ 1005 in the constellationCetus |
GJ 1005 is a system of twored dwarfs, located inconstellationCetus at 19.6light-years fromEarth.[7] The primary star is a M4Vclass star while the secondary is a class M7V.[citation needed]
The system was observed with theHubble Space Telescope in the 1990s with itsFine Guidance Sensor.[7] This data helped determine the mass of each of the components of L722-22/ LHS 1047 / GJ 1005.[7]