Taygeta
Star Taygeta (19 Tauri) |
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Above right in the Pleiades: Taygeta | |||||||||||||||||||||
AladinLite | |||||||||||||||||||||
Observation dates equinox : J2000.0 , epoch : J2000.0 |
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Constellation | bull | ||||||||||||||||||||
Right ascension | 03 h 45 m 12.5 s | ||||||||||||||||||||
declination | + 24 ° 28 ′ 2.2 ″ | ||||||||||||||||||||
Apparent brightness | 4.30 mag | ||||||||||||||||||||
Typing | |||||||||||||||||||||
B − V color index | (−0.11) | ||||||||||||||||||||
U − B color index | (−0.46) | ||||||||||||||||||||
R − I index | (−0.10) | ||||||||||||||||||||
Spectral class | B6 IV | ||||||||||||||||||||
Variable star type | SPB | ||||||||||||||||||||
Astrometry | |||||||||||||||||||||
Radial velocity | (7.8 ± 0.6) km / s | ||||||||||||||||||||
parallax | (8.97 ± 0.40) mas | ||||||||||||||||||||
distance | (364 ± 16) ly (111 ± 5) pc |
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Visual absolute brightness M vis | −1.62 mag | ||||||||||||||||||||
Proper movement | |||||||||||||||||||||
Rec. Share: | (21.24 ± 0.38) mas / a | ||||||||||||||||||||
Dec. portion: | (−40.56 ± 0.35) mas / a | ||||||||||||||||||||
Physical Properties | |||||||||||||||||||||
Dimensions | (4.41 ± 0.09) M ☉ | ||||||||||||||||||||
radius | (4.36 ± 0.14) R ☉ | ||||||||||||||||||||
Effective temperature | (13696 ± 222) K. | ||||||||||||||||||||
Other names and catalog entries |
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Taygeta (also Tayeta , one of the seven daughters of Atlas and Pleione , the Pleiades ) is the proper name of the star 19 Tauri in the Pleiades .
Taygeta, like all stars of the Pleiades, can occasionally be covered by the moon .
Taygeta has an apparent magnitude of +4.30 mag and belongs to the spectral class B6IV. Taygeta is a little over 360 light-years from Earth, whereby the distance, as with all Pleiades, is still afflicted with a relatively large error. The star is changeable and belongs to the star class of slowly pulsating B stars .
Web links
- Taygeta in Jim Kaler's star catalog
Individual evidence
- ↑ a b c d Gaia data release 2 ( Gaia DR2 ), April 2018
- ^ Hipparcos catalog (ESA 1997)
- ↑ a b c d e q Tau. In: SIMBAD . Center de Données astronomiques de Strasbourg , accessed July 22, 2018 .
- ↑ a b NSV 1264. In: VSX. AAVSO, accessed July 22, 2018 .
- ^ Hipparcos, the New Reduction (van Leeuwen, 2007)
- ↑ a b c TR White, BJS Pope, V. Antoci, PI Pápics, C. Aerts, DR Gies, K. Gordon, D. Huber, GH Schaefer, S. Aigrain, S. Albrecht, T. Barclay, G. Barentsen , PG Beck, TR Bedding, M. Fredslund Andersen, F. Grundahl, SB Howell, MJ Ireland, SJ Murphy, MB Nielsen, V. Silva Aguirre, PG Tuthill: Beyond the Kepler / K2 bright limit: Variability in the seven brightest members of the Pleiades . In: Monthly Notices of the Royal Astronomical Society . 471, No. 3, 2017, pp. 2882–2901. arxiv : 1708.07462 . bibcode : 2017MNRAS.471.2882W . doi : 10.1093 / mnras / stx1050 .