Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Pyxis |
Right ascension | 08h 40m 59.2056s[1] |
Declination | −23° 27′ 22.5986″[1] |
Apparent magnitude (V) | 11.98[2] |
Characteristics | |
Spectral type | M2.5V[3] |
V−R color index | 0.338[2] |
Astrometry | |
Radial velocity (Rv) | 87.8[3] km/s |
Proper motion (μ) | RA: −461.162±0.139 mas/yr[1] Dec.: 805.571±0.126 mas/yr[1] |
Parallax (π) | 65.7744 ± 0.0557 mas[1] |
Distance | 49.59 ± 0.04 ly (15.20 ± 0.01 pc) |
Absolute magnitude (MV) | 11.06±0.04[3] |
Details | |
Mass | 0.42±0.05[3] M☉ |
Radius | 0.4170±0.0013[4] R☉ |
Luminosity | 0.02175±0.00034[4] L☉ |
Temperature | 3,510±50[3] K |
Metallicity [Fe/H] | +0.3[3][5] dex |
Rotation | 69 days[6] |
Age | ~5[3] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Exoplanet Archive | data |
Gliese 317 is a small red dwarf star with two exoplanetary companions[3][8] in the southern constellation of Pyxis. It is located at a distance of 49.6 light-years from the Sun based on parallax measurements,[1] and is drifting further away with a radial velocity of +87.8 km/s.[3] This star is too faint to be viewed with the naked eye, having an apparent visual magnitude of 11.98[2] and an absolute magnitude of 11.06.[3]
This is an M-type main-sequence star with a stellar classification of M2.5V.[3] Photometric calibrations and infrared spectroscopic measurements indicate that the star is enriched in heavy elements compared to the Sun.[5] The star is estimated to be roughly five billion years old and has a low activity level for a star of its class.[3] It has 42%[3][4] of the mass and radius of the Sun and is spinning with a rotation period of 69 days.[6] The star is radiating 2.2%[4] of the Sun's luminosity from its photosphere at an effective temperature of 3,510 K.[3]
Gaia DR2
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