Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 14h 28m 12.13894s [1] |
Declination | −02° 13′ 40.6579″ [1] |
Apparent magnitude (V) | +4.81 [2] |
Characteristics | |
Spectral type | G2 IV [2] |
B−V color index | +0.683 [3] |
Astrometry | |
Radial velocity (Rv) | −9.88±0.15 [3] km/s |
Proper motion (μ) |
RA: −139.53
[1]
mas/
yr Dec.: −4.04 [1] mas/ yr |
Parallax (π) | 27.58 ± 1.01 mas [1] |
Distance | 118 ± 4
ly (36 ± 1 pc) |
Absolute magnitude (MV) | 1.68 [4] |
Details [3] | |
Mass | 1.80 [5] M☉ |
Radius | 4 R☉ |
Luminosity | 12.6 L☉ |
Surface gravity (log g) | 3.4 cgs |
Temperature | 5,534 K |
Metallicity [Fe/H] | −0.06 dex |
Rotational velocity (v sin i) | 15.5 km/s |
Age | 1.5 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Phi Virginis (φ Virginis, abbreviated Phi Vir, φ Vir) is a binary star [7] in the zodiac constellation of Virgo. It can be seen with the naked eye, having an apparent visual magnitude of +4.81. [2] Based upon parallax measurements obtained during the Hipparcos mission, it is located roughly 118 light-years (36 parsecs) distant from the Sun. [1]
The two components are designated Phi Virginis A (officially named Elgafar /ˈɛlɡəfɑːr/, the traditional name for the system) [8] and B.
φ Virginis ( Latinised to Phi Virginis) is the binary's Bayer designation. The designations of the two components as Phi Virginis A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). [9]
Ideler described an Arabic lunar mansion "El-ġafr" (Arabic الغفر al-ghafr) for the stars Phi, Iota and Kappa Virginis. [10] In 2016, the IAU organized a Working Group on Star Names (WGSN) [11] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. [12] It approved the name Elgafar for the component Phi Virginis A on 1 June 2018 and it is now so included in the List of IAU-approved Star Names. [8]
In Chinese, 亢宿 (Kàng Xiù), meaning Neck, refers to an asterism consisting of Phi Virginis, Kappa Virginis, Iota Virginis, and Lambda Virginis. [13] Consequently, Phi Virginis itself is known as 亢宿三 (Wěi Xiù sān), "the Third Star of Neck". [14]
The primary component, Phi Virginis A, has a stellar classification of G2 IV, [2] indicating that it is a G-type subgiant which is evolving away from the main sequence. It is slightly variable with an amplitude of 0m.06. [15] The star has about 1.8 times the mass of the Sun, [5] 4 times the Sun's radius, and shines with 12.6 times the luminosity of the Sun. [3] It is around 1.5 [5] billion years old and is spinning with a projected rotational velocity of 15.5 km/s. The effective temperature of the star's outer atmosphere is 5,534 K. [3]
The secondary, Phi Virginis B, is a magnitude 9.10 companion at an angular separation of 5.160 arcseconds. [7] A second visual companion lies at an angular separation of 91.40 arcseconds along a position angle of 202°, as of 2000. [16]
The system is a source of X-ray emission with a luminosity of 2.158×1020 erg/s. [17]
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Virgo |
Right ascension | 14h 28m 12.13894s [1] |
Declination | −02° 13′ 40.6579″ [1] |
Apparent magnitude (V) | +4.81 [2] |
Characteristics | |
Spectral type | G2 IV [2] |
B−V color index | +0.683 [3] |
Astrometry | |
Radial velocity (Rv) | −9.88±0.15 [3] km/s |
Proper motion (μ) |
RA: −139.53
[1]
mas/
yr Dec.: −4.04 [1] mas/ yr |
Parallax (π) | 27.58 ± 1.01 mas [1] |
Distance | 118 ± 4
ly (36 ± 1 pc) |
Absolute magnitude (MV) | 1.68 [4] |
Details [3] | |
Mass | 1.80 [5] M☉ |
Radius | 4 R☉ |
Luminosity | 12.6 L☉ |
Surface gravity (log g) | 3.4 cgs |
Temperature | 5,534 K |
Metallicity [Fe/H] | −0.06 dex |
Rotational velocity (v sin i) | 15.5 km/s |
Age | 1.5 [5] Gyr |
Other designations | |
Database references | |
SIMBAD | data |
Phi Virginis (φ Virginis, abbreviated Phi Vir, φ Vir) is a binary star [7] in the zodiac constellation of Virgo. It can be seen with the naked eye, having an apparent visual magnitude of +4.81. [2] Based upon parallax measurements obtained during the Hipparcos mission, it is located roughly 118 light-years (36 parsecs) distant from the Sun. [1]
The two components are designated Phi Virginis A (officially named Elgafar /ˈɛlɡəfɑːr/, the traditional name for the system) [8] and B.
φ Virginis ( Latinised to Phi Virginis) is the binary's Bayer designation. The designations of the two components as Phi Virginis A and B derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). [9]
Ideler described an Arabic lunar mansion "El-ġafr" (Arabic الغفر al-ghafr) for the stars Phi, Iota and Kappa Virginis. [10] In 2016, the IAU organized a Working Group on Star Names (WGSN) [11] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. [12] It approved the name Elgafar for the component Phi Virginis A on 1 June 2018 and it is now so included in the List of IAU-approved Star Names. [8]
In Chinese, 亢宿 (Kàng Xiù), meaning Neck, refers to an asterism consisting of Phi Virginis, Kappa Virginis, Iota Virginis, and Lambda Virginis. [13] Consequently, Phi Virginis itself is known as 亢宿三 (Wěi Xiù sān), "the Third Star of Neck". [14]
The primary component, Phi Virginis A, has a stellar classification of G2 IV, [2] indicating that it is a G-type subgiant which is evolving away from the main sequence. It is slightly variable with an amplitude of 0m.06. [15] The star has about 1.8 times the mass of the Sun, [5] 4 times the Sun's radius, and shines with 12.6 times the luminosity of the Sun. [3] It is around 1.5 [5] billion years old and is spinning with a projected rotational velocity of 15.5 km/s. The effective temperature of the star's outer atmosphere is 5,534 K. [3]
The secondary, Phi Virginis B, is a magnitude 9.10 companion at an angular separation of 5.160 arcseconds. [7] A second visual companion lies at an angular separation of 91.40 arcseconds along a position angle of 202°, as of 2000. [16]
The system is a source of X-ray emission with a luminosity of 2.158×1020 erg/s. [17]