Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 17h 10m 10.35091s [1] |
Declination | −60° 43′ 43.5757″ [1] |
Apparent magnitude (V) | 7.385 [2] |
Characteristics | |
Spectral type | K2.5Vk: [3] |
U−B color index | +0.53 [4] |
B−V color index | +0.89 [4] |
Astrometry | |
Radial velocity (Rv) | +8.8 [5] km/s |
Proper motion (μ) |
RA: 70.96
[1]
mas/
yr Dec.: 589.86 [1] mas/ yr |
Parallax (π) | 73.41 ± 0.70 mas [1] |
Distance | 44.4 ± 0.4
ly (13.6 ± 0.1 pc) |
Absolute magnitude (MV) | 6.71 [2] |
Details | |
Mass | 0.68 [6] M☉ |
Radius | 0.68 [7] R☉ |
Luminosity | 0.24 [8] L☉ |
Surface gravity (log g) | 4.70 [3] cgs |
Temperature | 4,850 [3] K |
Metallicity [Fe/H] | −0.70 [9] dex |
Rotational velocity (v sin i) | 0.2 [10] km/s |
Age | 3.2 [11] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
ARICNS | data |
HD 154577 (Gliese 656) is a solar-type star in the southern constellation of Ara. It is a high proper motion star and, based upon an annual parallax shift of 73.41 mas, [1] is located about 44 light years from the Sun. The star is too faint to be readily visible to the naked eye, having an apparent visual magnitude of 7.4. [2] It is moving away from the Sun with a radial velocity of +9 km/s. [5]
This star has only 68% of the Sun's mass and radius, an effective temperature of 4,850 K and a stellar classification of K2.5Vk:, [3] which indicates it is a K-type main sequence star. (The 'k' suffix indicates there are interstellar absorption features in the spectra, while ':' means there is some uncertainty about the classification.) It is about 3.2 [11] billion years old and appears to be spinning slowly with a projected rotational velocity of 0.2 km/s. [10] The star is radiating 24% [8] of the Sun's luminosity from its photosphere at an effective temperature of 4,850 K. [3]
As of 2005, this star is not known to host any planets. [6] No excess of infrared radiation has been detected of the type that would indicate the presence of an orbiting debris disk. [11]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Ara |
Right ascension | 17h 10m 10.35091s [1] |
Declination | −60° 43′ 43.5757″ [1] |
Apparent magnitude (V) | 7.385 [2] |
Characteristics | |
Spectral type | K2.5Vk: [3] |
U−B color index | +0.53 [4] |
B−V color index | +0.89 [4] |
Astrometry | |
Radial velocity (Rv) | +8.8 [5] km/s |
Proper motion (μ) |
RA: 70.96
[1]
mas/
yr Dec.: 589.86 [1] mas/ yr |
Parallax (π) | 73.41 ± 0.70 mas [1] |
Distance | 44.4 ± 0.4
ly (13.6 ± 0.1 pc) |
Absolute magnitude (MV) | 6.71 [2] |
Details | |
Mass | 0.68 [6] M☉ |
Radius | 0.68 [7] R☉ |
Luminosity | 0.24 [8] L☉ |
Surface gravity (log g) | 4.70 [3] cgs |
Temperature | 4,850 [3] K |
Metallicity [Fe/H] | −0.70 [9] dex |
Rotational velocity (v sin i) | 0.2 [10] km/s |
Age | 3.2 [11] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
ARICNS | data |
HD 154577 (Gliese 656) is a solar-type star in the southern constellation of Ara. It is a high proper motion star and, based upon an annual parallax shift of 73.41 mas, [1] is located about 44 light years from the Sun. The star is too faint to be readily visible to the naked eye, having an apparent visual magnitude of 7.4. [2] It is moving away from the Sun with a radial velocity of +9 km/s. [5]
This star has only 68% of the Sun's mass and radius, an effective temperature of 4,850 K and a stellar classification of K2.5Vk:, [3] which indicates it is a K-type main sequence star. (The 'k' suffix indicates there are interstellar absorption features in the spectra, while ':' means there is some uncertainty about the classification.) It is about 3.2 [11] billion years old and appears to be spinning slowly with a projected rotational velocity of 0.2 km/s. [10] The star is radiating 24% [8] of the Sun's luminosity from its photosphere at an effective temperature of 4,850 K. [3]
As of 2005, this star is not known to host any planets. [6] No excess of infrared radiation has been detected of the type that would indicate the presence of an orbiting debris disk. [11]