Astronomy:90 Tauri
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Short description: A-type main-sequence star in the constellation Taurus
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Taurus |
| Right ascension | 04h 38m 09.46166s[1] |
| Declination | +12° 30′ 38.9918″[1] |
| Apparent magnitude (V) | 4.27[2] |
| Characteristics | |
| Spectral type | A6 V[3] |
| U−B color index | +0.11[4] |
| B−V color index | +0.12[4] |
| Astrometry | |
| Radial velocity (Rv) | 40.30±1[5] km/s |
| Proper motion (μ) | RA: 102.40[6] mas/yr Dec.: −15.78[6] mas/yr |
| Parallax (π) | 22.6374 ± 0.3453[1] mas |
| Distance | 144 ± 2 ly (44.2 ± 0.7 pc) |
| Absolute magnitude (MV) | +1.18[7] |
| Details | |
| Mass | 2.09±0.11[8] M☉ |
| Radius | 2.8[8] R☉ |
| Surface gravity (log g) | 3.88±0.10[8] cgs |
| Temperature | 8,130[8] K |
| Rotational velocity (v sin i) | 89[3] km/s |
| Other designations | |
| Database references | |
| SIMBAD | data |
90 Tauri (90 Tau) is a star in the zodiac constellation of Taurus,[9] located 144 light-years away from the Sun.[1] It is visible to the naked eye as a faint, white-hued star with an apparent visual magnitude of 4.27.[2] 90 Tauri is a member of the Hyades cluster and is listed as a double star.
This is an A-type main-sequence star with a stellar classification of A6 V.[3] It has 2.1 times the mass of the Sun and 2.8 times the Sun's radius.[8] An orbiting companion was announced in 2014. This is probably a spectral class K4V star with an estimated orbital period of at least 84 days. The primary is being orbited by a debris disk.[10]
References
- ↑ 1.0 1.1 1.2 1.3 Brown, A. G. A. (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics 616: A1. doi:10.1051/0004-6361/201833051. Bibcode: 2018A&A...616A...1G. Gaia DR2 record for this source at VizieR.
- ↑ 2.0 2.1 Ducati, J. R. (2002). "VizieR Online Data Catalog: Catalogue of Stellar Photometry in Johnson's 11-color system". CDS/ADC Collection of Electronic Catalogues 2237. Bibcode: 2002yCat.2237....0D.
- ↑ 3.0 3.1 3.2 Royer, F.; Zorec, J.; Gómez, A. E. (2007). "Rotational velocities of A-type stars". Astronomy and Astrophysics 463 (2): 671. doi:10.1051/0004-6361:20065224. Bibcode: 2007A&A...463..671R.
- ↑ 4.0 4.1 Mermilliod, J.-C. (1986). "Compilation of Eggen's UBV data, transformed to UBV (unpublished)". Catalogue of Eggen's UBV Data. Bibcode: 1986EgUBV........0M.
- ↑ Gontcharov, G. A. (2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters 32 (11): 759–771. doi:10.1134/S1063773706110065. Bibcode: 2006AstL...32..759G.
- ↑ 6.0 6.1 van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics 474 (2): 653–664. doi:10.1051/0004-6361:20078357. Bibcode: 2007A&A...474..653V.
- ↑ Eggen, Olin J. (July 1998), "The Age Range of Hyades Stars", The Astronomical Journal 116 (1): 284–292, doi:10.1086/300413, Bibcode: 1998AJ....116..284E.
- ↑ 8.0 8.1 8.2 8.3 8.4 Allende Prieto, C.; Lambert, D. L. (1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics 352: 555–562. Bibcode: 1999A&A...352..555A.
- ↑ 9.0 9.1 "90 Tau". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=90+Tau.
- ↑ Marion, L. et al. (October 2014), "Searching for faint companions with VLTI/PIONIER. II. 92 main sequence stars from the Exozodi survey", Astronomy & Astrophysics 570: 12, doi:10.1051/0004-6361/201424780, A127, Bibcode: 2014A&A...570A.127M.
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