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Eta Volantis
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  | |
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Volans |
| Right ascension | 08h 22m 04.45155s[1] |
| Declination | −73° 23′ 59.9258″[1] |
| Apparent magnitude (V) | 5.28±0.01 |
| Characteristics | |
| Evolutionary stage | main sequence[2] |
| Spectral type | A0/1 IV/V[3] |
| B−V color index | +0.01[4] |
| Astrometry | |
| Radial velocity (Rv) | +20.0±3.7[5] km/s |
| Proper motion (μ) | RA: −29.432[1] mas/yr Dec.: +29.926[1] mas/yr |
| Parallax (π) | 8.4310±0.0887 mas[1] |
| Distance | 387 ± 4 ly (119 ± 1 pc) |
| Absolute magnitude (MV) | −0.06[6] |
| Details | |
| Mass | 2.73±0.08[7] M☉ |
| Radius | 3.78±0.12[8] R☉ |
| Luminosity | 84[9] L☉ |
| Surface gravity (log g) | 3.81±0.04[7] cgs |
| Temperature | 9,789±427[10] K |
| Rotational velocity (v sin i) | 214[11] km/s |
| Age | 347[7] Myr |
| Other designations | |
| η Vol, CPD−72°694, FK5 2653, HD 71576, HIP 41003, HR 3334, SAO 256505[12] | |
| Database references | |
| SIMBAD | data |
Eta Volantis, Latinized from η Volantis, is a single star[13] in the southern constellation of Volans. It has an apparent visual magnitude of 5.28,[14] which is bright enough to be seen with the naked eye as a dim, white-hued star. Based upon parallax measurements, it is approximately 387 light years from the Sun. The star is moving further away from the Sun with a radial velocity of 20 km/s.[5]
This is an A-type star with a stellar classification of A0/1 IV/V,[3] displaying blended spectrum that shows aspects of a main sequence star and a subgiant. Stellar evolution models from Zorec and Royer (2012) place it on the main sequence turnoff, having completed 90.7% of its time on the main sequence.[2] The star is estimated to be 347 million years old[7] and is spinning rapidly with a projected rotational velocity of 214 km/s.[11] It has 2.73 times the mass of the Sun[7] and 3.43 times the Sun's radius.[8] Eta Volantis is radiating 84[9] times the luminosity of the Sun from its photosphere at an effective temperature of 9,789 K.[10]
Eta Volantis has two 12th magnitude optical companions at angular separations of 26.8 and 48.1 arcseconds.[15]
References
[edit]- ^ a b c d e Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ a b Zorec, J.; Royer, F. (2012). "Rotational velocities of A-type stars. IV. Evolution of rotational velocities". Astronomy and Astrophysics. 537: A120. arXiv:1201.2052. Bibcode:2012A&A...537A.120Z. doi:10.1051/0004-6361/201117691.
- ^ a b Houk, N.; Cowley, A. P. (1975). University of Michigan Catalogue of two-dimensional spectral types for the HD stars. Volume I. Declinations −90° to −53°. Bibcode:1975mcts.book.....H.
- ^ Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data. SIMBAD, Bibcode:1986EgUBV........0M.
- ^ a b Kharchenko, N. V.; et al. (2007), "Astrophysical supplements to the ASCC-2.5: Ia. Radial velocities of ˜55000 stars and mean radial velocities of 516 Galactic open clusters and associations", Astronomische Nachrichten, 328 (9): 889, arXiv:0705.0878, Bibcode:2007AN....328..889K, doi:10.1002/asna.200710776, S2CID 119323941.
- ^ Anderson, E.; Francis, Ch. (May 2012). "XHIP: An extended hipparcos compilation". Astronomy Letters. 38 (5): 331–346. arXiv:1108.4971. Bibcode:2012AstL...38..331A. doi:10.1134/S1063773712050015. eISSN 1562-6873. ISSN 1063-7737. S2CID 119257644.
- ^ a b c d e Gerbaldi, M.; Faraggiana, R.; Burnage, R.; Delmas, F.; Gómez, A. E.; Grenier, S. (June 1999). "Search for reference A0 dwarf stars: Masses and luminosities revisited withHipparcos parallaxes". Astronomy and Astrophysics Supplement Series. 137 (2): 273–292. Bibcode:1999A&AS..137..273G. doi:10.1051/aas:1999248. eISSN 1286-4846. ISSN 0365-0138.
- ^ a b Stassun, Keivan G.; et al. (9 September 2019). "The Revised TESS Input Catalog and Candidate Target List". The Astronomical Journal. 158 (4): 138. arXiv:1905.10694. Bibcode:2019AJ....158..138S. doi:10.3847/1538-3881/ab3467. eISSN 1538-3881.
- ^ a b McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (2012). "Fundamental Parameters and Infrared Excesses of Hipparcos Stars". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–57. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. S2CID 118665352.
- ^ a b Paunzen, E.; Schnell, A.; Maitzen, H. M. (October 2006). "An empirical temperature calibration for the Δa photometric system II: The A-type and mid F-type stars". Astronomy & Astrophysics. 458 (1): 293–296. arXiv:astro-ph/0607567. Bibcode:2006A&A...458..293P. doi:10.1051/0004-6361:20064889. eISSN 1432-0746. ISSN 0004-6361.
- ^ a b Royer, F.; et al. (February 2007), "Rotational velocities of A-type stars. III. Velocity distributions", Astronomy and Astrophysics, 463 (2): 671–682, arXiv:astro-ph/0610785, Bibcode:2007A&A...463..671R, doi:10.1051/0004-6361:20065224, S2CID 18475298.
- ^ "* eps Vol". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2016-09-02.
{{cite web}}: CS1 maint: postscript (link) - ^ 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, arXiv:0806.2878, Bibcode:2008MNRAS.389..869E, doi:10.1111/j.1365-2966.2008.13596.x, S2CID 14878976.
- ^ Høg, E.; Fabricius, C.; Makarov, V. V.; Urban, S.; Corbin, T.; Wycoff, G.; Bastian, U.; Schwekendiek, P.; Wicenec, A. (March 2000). "The Tycho-2 catalogue of the 2.5 million brightest stars". Astronomy and Astrophysics. 355: L27–L30. Bibcode:2000A&A...355L..27H. ISSN 0004-6361.
- ^ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466, Bibcode:2001AJ....122.3466M, doi:10.1086/323920
