HD 64484
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Volans |
Right ascension | 07h 49m 40.9911s[1] |
Declination | −66° 11′ 45.5045″[1] |
Apparent magnitude (V) | 5.76±0.01[2] |
Characteristics | |
Evolutionary stage | main sequence[3] |
Spectral type | B9 V[4] |
U−B color index | −0.16[5] |
B−V color index | −0.04[5] |
Astrometry | |
Radial velocity (Rv) | 11±4.3[6] km/s |
Proper motion (μ) | RA: −2.037 mas/yr[1] Dec.: −0.411 mas/yr[1] |
Parallax (π) | 7.1191 ± 0.0628 mas[1] |
Distance | 458 ± 4 ly (140 ± 1 pc) |
Absolute magnitude (MV) | −0.11[7] |
Details | |
Mass | 2.80±0.13[8] M☉ |
Radius | 3.3±0.3[8] R☉ |
Luminosity | 140±8[3] L☉ |
Surface gravity (log g) | 3.86±0.06[9] cgs |
Temperature | 10,544±48[3] K |
Metallicity [Fe/H] | 0.00[10] dex |
Rotational velocity (v sin i) | 154[11] km/s |
Age | 339+50 −44[8] Myr |
Other designations | |
Database references | |
SIMBAD | data |
HD 64484 (HR 3081) is a solitary[12] star in the southern circumpolar constellation Volans. With an apparent magnitude of 5.76,[2] it is faintly visible to the naked eye under dark skies. Parallax measurements place it at a distance of 458 light years[1] but is receding with a heliocentric radial velocity of 11 km/s.[6]
HD 64484 has a stellar classification of B9 V,[4] indicating that it is an ordinary B-type main-sequence star. It has 2.8 times the mass of the Sun[8] and an effective temperature of 10,544 K,[3] giving it a bluish white hue. However, a slightly enlarged radius of 3.3 R☉[8] yields a luminosity 140 times that of the Sun.[3] This is due to HD 64484 completing 80.6% of its main sequence[3] lifetime at an age of 339 million years.[8] The star has a solar metallicity[10] and like many hot stars — spins rapidly with a projected rotational velocity of 154 km/s.[11]
References
[edit]- ^ a b c d e Brown, A. G. A.; et al. (Gaia collaboration) (2021). "Gaia Early Data Release 3: Summary of the contents and survey properties". Astronomy & Astrophysics. 649: A1. arXiv:2012.01533. Bibcode:2021A&A...649A...1G. doi:10.1051/0004-6361/202039657. S2CID 227254300. (Erratum: doi:10.1051/0004-6361/202039657e). Gaia EDR3 record for this source at VizieR.
- ^ a b 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.
- ^ a b c d e f Zorec, J.; Royer, F. (January 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. ISSN 0004-6361. S2CID 55586789.
- ^ 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_ƒ0. Bibcode:1975mcts.book.....H.
- ^ a b Johnson, H. L.; Mitchell, R. I.; Iriarte, B.; Wisniewski, W. Z. (1966). "UBVRIJKL Photometry of the Bright Stars". Communications of the Lunar and Planetary Laboratory. 4: 99–110. Bibcode:1966CoLPL...4...99J.
- ^ a b Gontcharov, G. A. (November 2006). "Pulkovo Compilation of Radial Velocities for 35 495 Hipparcos stars in a common system". Astronomy Letters. 32 (11): 759–771. arXiv:1606.08053. Bibcode:2006AstL...32..759G. doi:10.1134/S1063773706110065. ISSN 1063-7737. S2CID 119231169.
- ^ 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. ISSN 1063-7737. S2CID 255204555.
- ^ a b c d e f Bochanski, John J.; Faherty, Jacqueline K.; Gagné, Jonathan; Nelson, Olivia; Coker, Kristina; Smithka, Iliya; Desir, Deion; Vasquez, Chelsea (13 March 2018). "Fundamental Properties of Co-moving Stars Observed by Gaia". The Astronomical Journal. 155 (4): 149. arXiv:1801.00537. Bibcode:2018AJ....155..149B. doi:10.3847/1538-3881/aaaebe. ISSN 0004-6256. S2CID 119256051.
- ^ 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. ISSN 0004-6256.
- ^ a b Gontcharov, G. A. (December 2012). "Dependence of kinematics on the age of stars in the solar neighborhood". Astronomy Letters. 38 (12): 771–782. arXiv:1606.08814. Bibcode:2012AstL...38..771G. doi:10.1134/S1063773712120031. ISSN 0320-0108. S2CID 255201789.
- ^ a b Levato, H.; Grosso, M. (June 2004). "New Projected Rotational Velocities of All Southern B-type Stars of the Bright Star Catalogue". Astronomical Society of the Pacific. 215: 51. Bibcode:2004IAUS..215...51L.
- ^ 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.