Astronomy:Lambda1 Tucanae
From HandWiki
Short description: Binary star system in the constellation Tucana
| Observation data {{#ifeq:J2000.0|J2000.0 (ICRS)|Epoch J2000.0 Equinox J2000.0 (ICRS)| Epoch J2000.0 [[Astronomy:Equinox (celestial coordinates)|Equinox J2000.0}} | |
|---|---|
| Constellation | Tucana |
| A | |
| Right ascension | 00h 52m 24.5198s[1] |
| Declination | −69° 30′ 13.5440″[1] |
| Apparent magnitude (V) | 6.70[2] |
| B | |
| Right ascension | 00h 52m 28.3487s[3] |
| Declination | −69° 30′ 10.3819″[3] |
| Apparent magnitude (V) | 7.35[2] |
| Characteristics | |
| A | |
| Spectral type | F7 IV-V[4] |
| U−B color index | +0.07[5] |
| B−V color index | +0.55[5] |
| B | |
| Spectral type | G0/2V[4] |
| Astrometry | |
| A | |
| Radial velocity (Rv) | +29.4±0.2[6] km/s |
| Proper motion (μ) | RA: 3.849±0.050[1] mas/yr Dec.: −67.462±0.040[1] mas/yr |
| Parallax (π) | 16.4907 ± 0.0293[1] mas |
| Distance | 197.8 ± 0.4 ly (60.6 ± 0.1 pc) |
| Absolute magnitude (MV) | +2.68[7] |
| B | |
| Proper motion (μ) | RA: 9.966±0.062[3] mas/yr Dec.: −79.096±0.052[3] mas/yr |
| Parallax (π) | 16.5242 ± 0.0361[3] mas |
| Distance | 197.4 ± 0.4 ly (60.5 ± 0.1 pc) |
| Details | |
| A | |
| Mass | 1.55[8] M☉ |
| Luminosity | 7[9] L☉ |
| Surface gravity (log g) | 3.90[10] cgs |
| Temperature | 6,325[10] K |
| Metallicity [Fe/H] | +0.09[10] dex |
| Age | 2.6[10] Gyr |
| B | |
| Mass | 1.38[8] M☉ |
| Radius | 1.86[3] R☉ |
| Luminosity | 3.534[3] L☉ |
| Surface gravity (log g) | 3.94[11] cgs |
| Temperature | 5,797[3] K |
| Rotational velocity (v sin i) | 3.6[12] km/s |
| Other designations | |
| A: λ1 Tucanae, CPD−70 37, HD 5190, HIP 4084, HR 252, SAO 248269[13] | |
| B: CPD−70 38, HD 5208, HIP 4088, SAO 248271[13] | |
| Database references | |
| SIMBAD | data |
| companion | |
Lambda1 Tucanae is the Bayer designation for one member of a pair of stars sharing a common proper motion through space,[8] which lie within the southern constellation of Tucana. As of 2013, the pair had an angular separation of 20.0 arc seconds along a position angle of 82°.[2] Together, they are barely visible to the naked eye with a combined apparent visual magnitude of 6.21.[5] Based upon an annual parallax shift for both stars of approximately 16.5[1][3] mas as seen from Earth, this system is located roughly 198 light years from the Sun.
The brighter member, component A, is a magnitude 6.70[2] F-type star with a stellar classification of F7 IV-V.[4] The luminosity class may indicate that, at the age of 2.6 billion years,[10] it is beginning to evolve away from the main sequence. It has an estimated 1.55[8] times the mass of the Sun and is radiating 7[9] times the solar luminosity from its photosphere at an effective temperature of 6,325 K.[10] The magnitude 7.35[2] companion, component B, has 1.38[8] times the mass of the Sun. If the pair are gravitationally bound, then their estimated orbital period is 27,000 years.[8]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 1.5 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 2.2 2.3 2.4 Mason, B. D. et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal 122 (6): 3466, doi:10.1086/323920, Bibcode: 2001AJ....122.3466M.
- ↑ 3.0 3.1 3.2 3.3 3.4 3.5 3.6 3.7 3.8 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.
- ↑ 4.0 4.1 4.2 Houk, Nancy (1979), Michigan catalogue of two-dimensional spectral types for the HD stars, 1, Ann Arbor, Michigan: Dept. of Astronomy, University of Michigan, Bibcode: 1978mcts.book.....H.
- ↑ 5.0 5.1 5.2 Cousins, A. W. J.; Lagerweij, H. C. (1971), "UBV Observations of Variable Stars", Monthly Notes of the Astronomical Society of Southern Africa 30: 12, Bibcode: 1971MNSSA..30...12C.
- ↑ de Bruijne, J. H. J.; Eilers, A.-C. (October 2012), "Radial velocities for the HIPPARCOS-Gaia Hundred-Thousand-Proper-Motion project", Astronomy & Astrophysics 546: 14, doi:10.1051/0004-6361/201219219, A61, Bibcode: 2012A&A...546A..61D.
- ↑ Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 8.0 8.1 8.2 8.3 8.4 8.5 Tokovinin, Andrei (2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal 147 (4): 14, doi:10.1088/0004-6256/147/4/87, 87, Bibcode: 2014AJ....147...87T.
- ↑ 9.0 9.1 McDonald, I. et al. (2012), "Fundamental Parameters and Infrared Excesses of Hipparcos Stars", Monthly Notices of the Royal Astronomical Society 427 (1): 343–57, doi:10.1111/j.1365-2966.2012.21873.x, Bibcode: 2012MNRAS.427..343M.
- ↑ 10.0 10.1 10.2 10.3 10.4 10.5 Casagrande, L. et al. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics 530 (A138): 21, doi:10.1051/0004-6361/201016276, Bibcode: 2011A&A...530A.138C.
- ↑ Casagrande, L.; Schönrich, R.; Asplund, M.; Cassisi, S.; Ramírez, I.; Meléndez, J.; Bensby, T.; Feltzing, S. (2011), "New constraints on the chemical evolution of the solar neighbourhood and Galactic disc(s). Improved astrophysical parameters for the Geneva-Copenhagen Survey", Astronomy & Astrophysics 530 (A138): 21, doi:10.1051/0004-6361/201016276, Bibcode: 2011A&A...530A.138C.
- ↑ Głȩbocki, R.; Gnaciński, P. (2005). "Systematic errors in the determination of stellar rotational velocities". 13th Cambridge Workshop on Cool Stars 560: 571. Bibcode: 2005ESASP.560..571G.
- ↑ 13.0 13.1 13.2 "Lambda1 Tucanae". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=Lambda1+Tucanae.
 |  |
