Astronomy:Eta Trianguli Australis
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Triangulum Australe |
| Right ascension | 16h 41m 23.10722s[1] |
| Declination | −68° 17′ 46.0412″[1] |
| Apparent magnitude (V) | +5.91[2] |
| Characteristics | |
| Spectral type | B7 V[3] or B7 IVe[4] |
| U−B color index | −0.42[2] |
| B−V color index | −0.08[2] |
| Astrometry | |
| Radial velocity (Rv) | −10.0±7.6[5] km/s |
| Proper motion (μ) | RA: −14.067[1] mas/yr Dec.: −11.535[1] mas/yr |
| Parallax (π) | 4.2679 ± 0.0842[1] mas |
| Distance | 760 ± 20 ly (234 ± 5 pc) |
| Absolute magnitude (MV) | −0.36[6] |
| Details[7] | |
| Mass | 3.76±0.12 M☉ |
| Luminosity | 318 L☉ |
| Temperature | 12,162 K |
| Rotational velocity (v sin i) | 234 km/s |
| Age | 199[6] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
Eta Trianguli Australis (η Trianguli Australis) is a solitary,[9] blue-white hued star in the southern constellation Triangulum Australe. It is sometimes given a superscript: η1 Trianguli Australis, though it is the only star that is commonly referred to by this Bayer designation. Lacaille named a close by star as Eta as well, which was inconsistently followed by Francis Baily, who used the name for the brighter or both stars in two different publications. Despite their faintness, Gould upheld their Bayer designation as they were closer than 25 degrees to the south celestial pole. The second Eta is now designated as HD 150550.[10]
This star is faintly visible to the naked eye with an apparent visual magnitude of +5.91.[2] Based upon an annual parallax shift of just 4.93 mas as seen from the Earth, it is located roughly 760 light years from the Sun. At that distance, the visual magnitude of the star is diminished by an extinction of 0.28 due to interstellar dust.[6] The system appears to be moving closer to the Sun with a radial velocity of around −10 km/s.[5]
Eta Trianguli Australis is a B-type main-sequence star with a stellar classification of B7 V.[3] Although it has been classified as a B7 IVe Be subgiant star in the past,[4] Jaschek and Jaschek (1992) found no trace of emission in the spectrum.[11] Grady et al. (1989) reported only "weak or narrow double-peaked Hα emission, but no emission at Hβ".[12] The star shows a relatively high peculiar velocity of 40±20 km/s.[4] It is spinning rapidly with a projected rotational velocity of 234 km/s.[7]
References
- ↑ 1.0 1.1 1.2 1.3 1.4 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 Johnson, H. L. et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory 4 (99): 99, Bibcode: 1966CoLPL...4...99J.
- ↑ 3.0 3.1 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.
- ↑ 4.0 4.1 4.2 Berger, D. H.; Gies, D. R. (July 2001), "A Search for High-Velocity Be Stars", The Astrophysical Journal 555 (1): 364–367, doi:10.1086/321461, Bibcode: 2001ApJ...555..364B.
- ↑ 5.0 5.1 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.
- ↑ 6.0 6.1 6.2 Gontcharov, G. A. (November 2012), "Spatial distribution and kinematics of OB stars", Astronomy Letters 38 (11): 694–706, doi:10.1134/S1063773712110035, Bibcode: 2012AstL...38..694G.
- ↑ 7.0 7.1 Zorec, J.; Royer, F. (January 2012), "Rotational velocities of A-type stars. IV. Evolution of rotational velocities", Astronomy & Astrophysics 537: A120, doi:10.1051/0004-6361/201117691, Bibcode: 2012A&A...537A.120Z.
- ↑ "eta01 TrA". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=eta01+TrA.
- ↑ Eggleton, P. P.; Tokovinin, A. A. (September 2008), "A catalogue of multiplicity among bright stellar systems", Monthly Notices of the Royal Astronomical Society 389 (2): 869–879, doi:10.1111/j.1365-2966.2008.13596.x, Bibcode: 2008MNRAS.389..869E.
- ↑ Wagman, Morton (2003), Lost Stars: Lost, Missing and Troublesome Stars from the Catalogues of Johannes Bayer, Nicholas Louis de Lacaille, John Flamsteed, and Sundry Others, Blacksburg, VA: The McDonald & Woodward Publishing Company, pp. 303–04, ISBN 978-0-939923-78-6, Bibcode: 2003lslm.book.....W
- ↑ Jaschek, C.; Jaschek, M. (November 1992), "A southern Be star survey - Spectra and envelope radii", Astronomy and Astrophysics Supplement Series 95 (3): 535–540, Bibcode: 1992A&AS...95..535J.
- ↑ Grady, C. A. et al. (April 1, 1989), "Highly ionized stellar winds in Be stars. II - Winds in B6-B9.5e stars", Astrophysical Journal, Part 1 339: 403–419, doi:10.1086/167306, Bibcode: 1989ApJ...339..403G.
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