HD 130458
Observation data Epoch J2000.0 Equinox J2000.0 (ICRS) | |
---|---|
Constellation | Apus |
A | |
Right ascension | 14h 53m 13.6598s[1] |
Declination | −73° 11′ 23.837″[1] |
Apparent magnitude (V) | 5.77±0.01[2] |
B | |
Right ascension | 14h 53m 14.0752s[3] |
Declination | −73° 11′ 25.2484″[3] |
Apparent magnitude (V) | 7.54±0.01[2] |
Characteristics | |
A | |
Evolutionary stage | Horizontal branch[4] |
Spectral type | G7 IIIa[5] (G8 IIb)[4] |
U−B color index | +0.42[6] |
B−V color index | +0.82[6] |
B | |
Spectral type | F9 IV[5] |
Astrometry | |
Radial velocity (Rv) | +31.4 ± 2.5[7] km/s |
Absolute magnitude (MV) | +0.58[8] |
A | |
Proper motion (μ) | RA: +15.901[1] mas/yr Dec.: +28.871[1] mas/yr |
Parallax (π) | 10.5077 ± 0.3522 mas[1] |
Distance | 310 ± 10 ly (95 ± 3 pc) |
B | |
Proper motion (μ) | RA: +20.669[3] mas/yr Dec.: +19.875[3] mas/yr |
Parallax (π) | 10.0654 ± 0.0476 mas[3] |
Distance | 324 ± 2 ly (99.4 ± 0.5 pc) |
Details | |
A | |
Mass | 1.5[9] M☉ |
Radius | 8.87[10] R☉ |
Luminosity | 54.7[11] L☉ |
Surface gravity (log g) | 2.65[9] cgs |
Temperature | 5194±124[10] K |
Metallicity [Fe/H] | −0.17[9] dex |
Rotational velocity (v sin i) | 3.6±1[12] km/s |
B | |
Mass | 1.41[9] M☉ |
Radius | 2.8[13] R☉ |
Luminosity | 7.5[14] L☉ |
Surface gravity (log g) | 3.96[9] cgs |
Temperature | 6,601[9] K |
Metallicity [Fe/H] | −0.18[9] dex |
Other designations | |
Database references | |
SIMBAD | data |
HD 130458 (HR 5520) is a double star[17] in the southern circumpolar constellation of Apus. The pair has a combined apparent magnitude of 5.8,[6] making it faintly visible to the naked eye under ideal conditions. Parallax measurements place the system 310-24 light years away[1] and it is receding with a heliocentric radial velocity of 31.4 km/s.[7]
The primary is a red giant with a stellar classification of G7 IIIa. It was earlier classified as G8 IIb, indicating a bright giant.The dimmer component has a stellar classification of F9 IV, indicating that it is an F-type subgiant evolving onto the red giant branch. As of 2008 , the pair has an angular separation of 2.167″.[17]
At present the primary has 1.5 times the mass of the Sun[9] but has expanded to 8.9[10] times its girth. It radiates at 55[11] times the luminosity of the Sun from its enlarged photosphere at an effective temperature 5,194 K,[10] which gives it a yellow glow. Currently it spins leisurely with a projected rotational velocity of 3.6 km/s,[12] common for giants. HD 130458A is believed to be on the horizontal branch.[4]
As for the secondary component, it has 1.4 times the mass of the Sun and an effective temperature of 6,601 K, giving a yellowish white hue. [9]
References
- ^ a b c d e f 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 Fabricius, C.; Høg, E.; Makarov, V. V.; Mason, B. D.; Wycoff, G. L.; Urban, S. E. (March 2002). "The Tycho double star catalogue". Astronomy & Astrophysics. 384 (1): 180–189. Bibcode:2002A&A...384..180F. doi:10.1051/0004-6361:20011822. ISSN 0004-6361.
- ^ 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 c Corbally, C. J.; Garrison, R. F. (August 1980). "New Spectral Classifications on the MK System for Visual Double Stars". Publications of the Astronomical Society of the Pacific. 92: 493. Bibcode:1980PASP...92..493C. doi:10.1086/130700. eISSN 1538-3873. ISSN 0004-6280.
- ^ a b Corbally, C. J. (August 1984). "Close visual binaries. I - MK classifications". The Astrophysical Journal Supplement Series. 55: 657. Bibcode:1984ApJS...55..657C. doi:10.1086/190973. eISSN 1538-4365. ISSN 0067-0049.
- ^ a b c 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
- ^ 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 g h i Anders, F.; et al. (August 2019). "Photo-astrometric distances, extinctions, and astrophysical parameters for Gaia DR2 stars brighter than G = 18". Astronomy & Astrophysics. 628: A94. arXiv:1904.11302. Bibcode:2019A&A...628A..94A. doi:10.1051/0004-6361/201935765. ISSN 0004-6361.
- ^ a b c d 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 McDonald, I.; Zijlstra, A. A.; Boyer, M. L. (21 November 2012). "Fundamental parameters and infrared excesses of Hipparcos stars: Parameters and IR excesses from Hipparcos". Monthly Notices of the Royal Astronomical Society. 427 (1): 343–357. arXiv:1208.2037. Bibcode:2012MNRAS.427..343M. doi:10.1111/j.1365-2966.2012.21873.x. ISSN 0035-8711.
- ^ a b De Medeiros, J. R.; Da Silva, J. R. P.; Maia, M. R. G. (20 October 2002). "The Rotation of Binary Systems with Evolved Components". The Astrophysical Journal. 578 (2): 943–950. arXiv:astro-ph/0207288. Bibcode:2002ApJ...578..943D. doi:10.1086/342613. eISSN 1538-4357. ISSN 0004-637X.
- ^ Montalto, M.; et al. (2021). "The all-sky PLATO input catalogue". Astronomy and Astrophysics. 653: A98. arXiv:2108.13712. Bibcode:2021A&A...653A..98M. doi:10.1051/0004-6361/202140717. S2CID 237363915.
- ^ Brown, A. G. A.; et al. (Gaia collaboration) (August 2018). "Gaia Data Release 2: Summary of the contents and survey properties". Astronomy & Astrophysics. 616. A1. arXiv:1804.09365. Bibcode:2018A&A...616A...1G. doi:10.1051/0004-6361/201833051. Gaia DR2 record for this source at VizieR.
- ^ Gould, Benjamin Apthorp (1878). "Uranometria Argentina : brillantez y posicion de las estrellas fijas, hasta la septima magnitud, comprendidas dentro de cien grados del polo austral : con atlas". Resultados del Observatorio Nacional Argentino. 1. Bibcode:1879RNAO....1.....G.
- ^ "HR+5520". SIMBAD. Centre de données astronomiques de Strasbourg.
- ^ a b 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.
External links
- Image HD 130458