Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Taurus |
θ1 Tauri | |
Right ascension | 04h 28m 34.49603s [1] |
Declination | +15° 57′ 43.8494″ [1] |
Apparent magnitude (V) | +3.84 |
θ2 Tauri | |
Right ascension | 04h 28m 39.74070s [1] |
Declination | +15° 52′ 15.1745″ [1] |
Apparent magnitude (V) | +3.35 - 3.42 [2] |
Characteristics | |
θ1 Tauri | |
Spectral type | G9 III Fe-0.5 [3] |
θ2 Tauri | |
Spectral type | A7 III [4] |
Variable type | δ Scuti [2] |
Astrometry | |
θ1 Tauri | |
Parallax (π) | 21.4183 ± 0.3731 mas [5] |
Distance | 152 ± 3
ly (46.7 ± 0.8 pc) |
Absolute magnitude (MV) | +0.416 [6] |
θ2 Tauri | |
Parallax (π) | 20.8354 ± 0.3731 mas [7] |
Distance | 157 ± 3
ly (48.0 ± 0.9 pc) |
Absolute magnitude (MV) | +0.30/+1.44 [8] |
Orbit [9] | |
Primary | A |
Companion | B |
Period (P) | 5,997 days |
Eccentricity (e) | 0.64 |
Semi-amplitude (K1) (primary) | 8.39 km/s |
Orbit [8] | |
Primary | Aa |
Companion | Ab |
Period (P) | 140.7302 days |
Semi-major axis (a) | 18.91″ |
Eccentricity (e) | 0.7360 |
Inclination (i) | 47.8° |
Semi-amplitude (K1) (primary) | 32.95 km/s |
Semi-amplitude (K2) (secondary) | 43.68 km/s |
Details | |
Aa | |
Mass | 2.86 [10] M☉ |
Radius | 4.4 [10] R☉ |
Luminosity | 59 [8] L☉ |
Surface gravity (log g) | 3.6 [10] cgs |
Temperature | 7,800 [10] K |
Rotational velocity (v sin i) | 68.4 [8] km/s |
Ab | |
Mass | 2.16 [10] M☉ |
Radius | 2.7 [10] R☉ |
Luminosity | 21 [8] L☉ |
Temperature | 7,800 [8] K |
Rotational velocity (v sin i) | 113 [8] km/s |
Age | 650 [8] Myr |
θ1 Tauri | |
Mass | 2.67 [11] M☉ |
Radius | 9.42±0.22 [12] R☉ |
Luminosity | 47.7±2.3 [12] L☉ |
Surface gravity (log g) | 3.21 [11] cgs |
Temperature | 4,940±55 [12] K |
Metallicity [Fe/H] | +0.14 [11] dex |
Rotational velocity (v sin i) | 1.40 [11] km/s |
Age | 510 [11] Myr |
Other designations | |
θ Tauri | |
θ1 Tauri: 77 Tauri, BD+15 631, HD 28307, HIP 20885, HR 1411, SAO 93955 | |
θ2 Tauri: Chamukuy, 78 Tauri, BD+15 632, HD 28319, HIP 20894, HR 1412, SAO 93957 | |
Database references | |
SIMBAD | θ1 Tauri |
θ2 Tauri |
Theta Tauri (θ Tauri, abbreviated Theta Tau, θ Tau) is a wide double star in the constellation of Taurus and a member of the Hyades open cluster.
θ Tauri is composed of two 3rd magnitude stars, designated Theta1 Tauri (Theta Tauri B) and Theta2 Tauri (Theta Tauri A). Theta² is brighter, hence the pair are sometimes referred to as Theta Tauri B and A, respectively. They are separated by 5.62 arcminutes (0.094°) on the sky. Based upon parallax measurements, Theta¹ Tauri is located at a distance of 152 ly (47 pc), while Theta² Tauri is at a distance of 157 light-years (48 parsecs). θ Tauri A and B are both spectroscopic binaries; the four components are designated Theta Tauri Aa (formally named Chamukuy /ˈtʃɑːmuːkuːi/), Ab, Ba, and Bb.
θ Tauri ( Latinised to Theta Tauri) is the double star's Bayer designation;[ citation needed] θ1 Tauri and θ2 Tauri those of its two constituents. The designations of the two constituents as Theta Tauri A and B, and those of the four components - Theta Tauri Aa, Ab, Ba and Bb - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). [13]
In the mythology of the Maya peoples, Theta Tauri is known as Chamukuy, meaning a small bird in the Yucatec Maya language. [14] In 2016, the IAU organized a Working Group on Star Names (WGSN) [15] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. [16] It approved the name Chamukuy for the component Theta Tauri Aa on 5 September 2017 and it is now so included in the List of IAU-approved Star Names. [17]
In Chinese, 畢宿 (Bì Xiù), meaning Net, refers to an asterism consisting of Theta² Tauri, Epsilon Tauri (named Ain), Delta³ Tauri, Delta¹ Tauri, Gamma Tauri, Alpha Tauri ( Aldebaran), 71 Tauri and Lambda Tauri. [18] Consequently, the Chinese name for Theta² Tauri itself is 畢宿六 (Bì Xiù liù), "the Sixth Star of Net". [19]
Theta Tauri A has a mean apparent magnitude of +3.40. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.35 to +3.42 with a period of 1.82 hours. [21] Its primary component, Theta Tauri Aa, is a white A-type giant. The secondary, Theta Tauri Ab, is of the 6th magnitude and is 0.005 arcseconds, or at least 2 AU, distant. It completes an orbit once every 141 days.
Theta Tauri B is the dimmer constituent. Its primary component, Theta Tauri Ba, is an orange K-type giant with an apparent magnitude of +3.84. The secondary, Theta Tauri Bb, is of the 7th-magnitude. It has a mass of 1.31 M☉ and orbits the primary every 16.26 years on a fairly eccentric (at 0.570) orbit. [22]
Observation data Epoch J2000.0 Equinox J2000.0 | |
---|---|
Constellation | Taurus |
θ1 Tauri | |
Right ascension | 04h 28m 34.49603s [1] |
Declination | +15° 57′ 43.8494″ [1] |
Apparent magnitude (V) | +3.84 |
θ2 Tauri | |
Right ascension | 04h 28m 39.74070s [1] |
Declination | +15° 52′ 15.1745″ [1] |
Apparent magnitude (V) | +3.35 - 3.42 [2] |
Characteristics | |
θ1 Tauri | |
Spectral type | G9 III Fe-0.5 [3] |
θ2 Tauri | |
Spectral type | A7 III [4] |
Variable type | δ Scuti [2] |
Astrometry | |
θ1 Tauri | |
Parallax (π) | 21.4183 ± 0.3731 mas [5] |
Distance | 152 ± 3
ly (46.7 ± 0.8 pc) |
Absolute magnitude (MV) | +0.416 [6] |
θ2 Tauri | |
Parallax (π) | 20.8354 ± 0.3731 mas [7] |
Distance | 157 ± 3
ly (48.0 ± 0.9 pc) |
Absolute magnitude (MV) | +0.30/+1.44 [8] |
Orbit [9] | |
Primary | A |
Companion | B |
Period (P) | 5,997 days |
Eccentricity (e) | 0.64 |
Semi-amplitude (K1) (primary) | 8.39 km/s |
Orbit [8] | |
Primary | Aa |
Companion | Ab |
Period (P) | 140.7302 days |
Semi-major axis (a) | 18.91″ |
Eccentricity (e) | 0.7360 |
Inclination (i) | 47.8° |
Semi-amplitude (K1) (primary) | 32.95 km/s |
Semi-amplitude (K2) (secondary) | 43.68 km/s |
Details | |
Aa | |
Mass | 2.86 [10] M☉ |
Radius | 4.4 [10] R☉ |
Luminosity | 59 [8] L☉ |
Surface gravity (log g) | 3.6 [10] cgs |
Temperature | 7,800 [10] K |
Rotational velocity (v sin i) | 68.4 [8] km/s |
Ab | |
Mass | 2.16 [10] M☉ |
Radius | 2.7 [10] R☉ |
Luminosity | 21 [8] L☉ |
Temperature | 7,800 [8] K |
Rotational velocity (v sin i) | 113 [8] km/s |
Age | 650 [8] Myr |
θ1 Tauri | |
Mass | 2.67 [11] M☉ |
Radius | 9.42±0.22 [12] R☉ |
Luminosity | 47.7±2.3 [12] L☉ |
Surface gravity (log g) | 3.21 [11] cgs |
Temperature | 4,940±55 [12] K |
Metallicity [Fe/H] | +0.14 [11] dex |
Rotational velocity (v sin i) | 1.40 [11] km/s |
Age | 510 [11] Myr |
Other designations | |
θ Tauri | |
θ1 Tauri: 77 Tauri, BD+15 631, HD 28307, HIP 20885, HR 1411, SAO 93955 | |
θ2 Tauri: Chamukuy, 78 Tauri, BD+15 632, HD 28319, HIP 20894, HR 1412, SAO 93957 | |
Database references | |
SIMBAD | θ1 Tauri |
θ2 Tauri |
Theta Tauri (θ Tauri, abbreviated Theta Tau, θ Tau) is a wide double star in the constellation of Taurus and a member of the Hyades open cluster.
θ Tauri is composed of two 3rd magnitude stars, designated Theta1 Tauri (Theta Tauri B) and Theta2 Tauri (Theta Tauri A). Theta² is brighter, hence the pair are sometimes referred to as Theta Tauri B and A, respectively. They are separated by 5.62 arcminutes (0.094°) on the sky. Based upon parallax measurements, Theta¹ Tauri is located at a distance of 152 ly (47 pc), while Theta² Tauri is at a distance of 157 light-years (48 parsecs). θ Tauri A and B are both spectroscopic binaries; the four components are designated Theta Tauri Aa (formally named Chamukuy /ˈtʃɑːmuːkuːi/), Ab, Ba, and Bb.
θ Tauri ( Latinised to Theta Tauri) is the double star's Bayer designation;[ citation needed] θ1 Tauri and θ2 Tauri those of its two constituents. The designations of the two constituents as Theta Tauri A and B, and those of the four components - Theta Tauri Aa, Ab, Ba and Bb - derive from the convention used by the Washington Multiplicity Catalog (WMC) for multiple star systems, and adopted by the International Astronomical Union (IAU). [13]
In the mythology of the Maya peoples, Theta Tauri is known as Chamukuy, meaning a small bird in the Yucatec Maya language. [14] In 2016, the IAU organized a Working Group on Star Names (WGSN) [15] to catalog and standardize proper names for stars. The WGSN decided to attribute proper names to individual stars rather than entire multiple systems. [16] It approved the name Chamukuy for the component Theta Tauri Aa on 5 September 2017 and it is now so included in the List of IAU-approved Star Names. [17]
In Chinese, 畢宿 (Bì Xiù), meaning Net, refers to an asterism consisting of Theta² Tauri, Epsilon Tauri (named Ain), Delta³ Tauri, Delta¹ Tauri, Gamma Tauri, Alpha Tauri ( Aldebaran), 71 Tauri and Lambda Tauri. [18] Consequently, the Chinese name for Theta² Tauri itself is 畢宿六 (Bì Xiù liù), "the Sixth Star of Net". [19]
Theta Tauri A has a mean apparent magnitude of +3.40. It is classified as a Delta Scuti type variable star and its brightness varies from magnitude +3.35 to +3.42 with a period of 1.82 hours. [21] Its primary component, Theta Tauri Aa, is a white A-type giant. The secondary, Theta Tauri Ab, is of the 6th magnitude and is 0.005 arcseconds, or at least 2 AU, distant. It completes an orbit once every 141 days.
Theta Tauri B is the dimmer constituent. Its primary component, Theta Tauri Ba, is an orange K-type giant with an apparent magnitude of +3.84. The secondary, Theta Tauri Bb, is of the 7th-magnitude. It has a mass of 1.31 M☉ and orbits the primary every 16.26 years on a fairly eccentric (at 0.570) orbit. [22]