Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Piscis Austrinus |
Right ascension | 22h 14m 18.75029s [1] |
Declination | −27° 46′ 00.8756″ [1] |
Apparent magnitude (V) | +5.42 [2] |
Characteristics | |
Spectral type | B7 V [3] |
B−V color index | −0.12 [2] |
Astrometry | |
Radial velocity (Rv) | −6.20 [4] km/s |
Proper motion (μ) |
RA: +23.889
[1]
mas/
yr Dec.: +2.562 [1] mas/ yr |
Parallax (π) | 6.5148 ± 0.2222 mas [1] |
Distance | 500 ± 20
ly (153 ± 5 pc) |
Absolute magnitude (MV) | −0.13 [5] |
Details | |
Mass | 3.58±0.08 [6] M☉ |
Radius | 4.2 [7] R☉ |
Luminosity | 249 [6] L☉ |
Temperature | 12,023 [6] K |
Rotational velocity (v sin i) | 50 [8] km/s |
Age | 215 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Lambda Piscis Austrini, Latinized from λ Piscis Austrini, is a solitary [10] star in the southern constellation of Piscis Austrinus. It has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +5.42. [2] Based upon an annual parallax shift of 6.51 mas as measured from Earth, [1] it is located around 500 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.16 due to interstellar dust. [5]
This is a B-type main sequence star with a stellar classification of B7 V. [3] It has an estimated 3.58 [6] times the mass of the Sun and about 4.2 [7] times the Sun's radius. The star is spinning with a projected rotational velocity of 50 km/s [8] and is 76% of the way through its main sequence lifetime. It is radiating 249 times the solar luminosity from its photosphere at an effective temperature of 12,023 K. [6]
Lambda Piscis Austrini is moving through the Galaxy at a speed of 18.1 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 29,300 light years from the center of the Galaxy. [11]
In Chinese, 羽林軍 (Yǔ Lín Jūn), meaning Palace Guard, refers to an asterism consisting of λ Piscis Austrini, 29 Aquarii, 35 Aquarii, 41 Aquarii, 47 Aquarii, 49 Aquarii, HD 212448, ε Piscis Austrini, 21 Piscis Austrini, 20 Piscis Austrini, υ Aquarii, 68 Aquarii, 66 Aquarii, 61 Aquarii, 53 Aquarii, 50 Aquarii, 56 Aquarii, 45 Aquarii, 58 Aquarii, 64 Aquarii, 65 Aquarii, 70 Aquarii, 74 Aquarii, τ2 Aquarii, τ1 Aquarii, δ Aquarii, 77 Aquarii, 88 Aquarii, 89 Aquarii, 86 Aquarii, 101 Aquarii, 100 Aquarii, 99 Aquarii, 98 Aquarii, 97 Aquarii, 94 Aquarii, ψ3Aquarii, ψ2Aquarii, ψ1Aquarii, 87 Aquarii, 85 Aquarii, 83 Aquarii, χ Aquarii, ω1 Aquarii and ω2 Aquarii. Consequently, the Chinese name for λ Piscis Austrini itself is 羽林軍六 (Yǔ Lín Jūn liù, English: the Sixth Star of Palace Guard.) [12]
Observation data Epoch J2000.0 Equinox J2000.0 ( ICRS) | |
---|---|
Constellation | Piscis Austrinus |
Right ascension | 22h 14m 18.75029s [1] |
Declination | −27° 46′ 00.8756″ [1] |
Apparent magnitude (V) | +5.42 [2] |
Characteristics | |
Spectral type | B7 V [3] |
B−V color index | −0.12 [2] |
Astrometry | |
Radial velocity (Rv) | −6.20 [4] km/s |
Proper motion (μ) |
RA: +23.889
[1]
mas/
yr Dec.: +2.562 [1] mas/ yr |
Parallax (π) | 6.5148 ± 0.2222 mas [1] |
Distance | 500 ± 20
ly (153 ± 5 pc) |
Absolute magnitude (MV) | −0.13 [5] |
Details | |
Mass | 3.58±0.08 [6] M☉ |
Radius | 4.2 [7] R☉ |
Luminosity | 249 [6] L☉ |
Temperature | 12,023 [6] K |
Rotational velocity (v sin i) | 50 [8] km/s |
Age | 215 [5] Myr |
Other designations | |
Database references | |
SIMBAD | data |
Lambda Piscis Austrini, Latinized from λ Piscis Austrini, is a solitary [10] star in the southern constellation of Piscis Austrinus. It has a blue-white hue and is visible to the naked eye with an apparent visual magnitude of +5.42. [2] Based upon an annual parallax shift of 6.51 mas as measured from Earth, [1] it is located around 500 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction factor of 0.16 due to interstellar dust. [5]
This is a B-type main sequence star with a stellar classification of B7 V. [3] It has an estimated 3.58 [6] times the mass of the Sun and about 4.2 [7] times the Sun's radius. The star is spinning with a projected rotational velocity of 50 km/s [8] and is 76% of the way through its main sequence lifetime. It is radiating 249 times the solar luminosity from its photosphere at an effective temperature of 12,023 K. [6]
Lambda Piscis Austrini is moving through the Galaxy at a speed of 18.1 km/s relative to the Sun. Its projected Galactic orbit carries it between 23,800 and 29,300 light years from the center of the Galaxy. [11]
In Chinese, 羽林軍 (Yǔ Lín Jūn), meaning Palace Guard, refers to an asterism consisting of λ Piscis Austrini, 29 Aquarii, 35 Aquarii, 41 Aquarii, 47 Aquarii, 49 Aquarii, HD 212448, ε Piscis Austrini, 21 Piscis Austrini, 20 Piscis Austrini, υ Aquarii, 68 Aquarii, 66 Aquarii, 61 Aquarii, 53 Aquarii, 50 Aquarii, 56 Aquarii, 45 Aquarii, 58 Aquarii, 64 Aquarii, 65 Aquarii, 70 Aquarii, 74 Aquarii, τ2 Aquarii, τ1 Aquarii, δ Aquarii, 77 Aquarii, 88 Aquarii, 89 Aquarii, 86 Aquarii, 101 Aquarii, 100 Aquarii, 99 Aquarii, 98 Aquarii, 97 Aquarii, 94 Aquarii, ψ3Aquarii, ψ2Aquarii, ψ1Aquarii, 87 Aquarii, 85 Aquarii, 83 Aquarii, χ Aquarii, ω1 Aquarii and ω2 Aquarii. Consequently, the Chinese name for λ Piscis Austrini itself is 羽林軍六 (Yǔ Lín Jūn liù, English: the Sixth Star of Palace Guard.) [12]