HD 130458
HD 130458 (HR 5520) is a double star[3] in the southern circumpolar constellation of Apus. The pair has a combined apparent magnitude of 5.8, making it faintly visible to the naked eye under ideal conditions. Currently located 330 light years away, HD 130458 is receding at a rate of 31.4 km/s.
Observation data Epoch J2000 Equinox J2000 | |
---|---|
Constellation | Apus |
Right ascension | 14h 53m 13.57117s[1] |
Declination | −73° 11′ 24.2613″[1] |
Apparent magnitude (V) | 5.80[2] (5.94 + 7.68)[3] |
Characteristics | |
Spectral type | G7IIIa + F9IV[3] |
U−B color index | +0.42[4] |
B−V color index | +0.82[4] |
Astrometry | |
Radial velocity (Rv) | +31.4 ± 2.5[5] km/s |
Proper motion (μ) | RA: 17.09±0.44[1] mas/yr Dec.: 33.78±0.49[1] mas/yr |
Parallax (π) | 9.90 ± 0.55 mas[1] |
Distance | 330 ± 20 ly (101 ± 6 pc) |
Absolute magnitude (MV) | +0.78 |
Details | |
Mass | 2.47 ± 0.13[6] M☉ |
Radius | 8.32+0.81 −0.73[6] R☉ |
Luminosity | 54.7[7] L☉ |
Surface gravity (log g) | 2.99 ± 0.10[6] cgs |
Temperature | 5,291[7] K |
Rotational velocity (v sin i) | 3.4[2] km/s |
Other designations | |
Database references | |
SIMBAD | data |
HD 130458 has a composite spectrum with a stellar classification of G7 IIIa + F9 IV.[3] This indicates that the primary is a late G-type giant star and the secondary a late F-type subgiant. At present the primary has 2.47[6] times the mass of the Sun but has expanded to 8.32[6] times its girth. It radiates at 55[7] times the luminosity of the Sun from its enlarged photosphere at an effective temperature 5,291 K,[7] which gives it a yellow glow. Currently it spins leisurely with a projected rotational velocity of 3.4 km/s,[2] common for giants. As of 2008 , the pair has an angular separation of 2.167″.[3]
References
- van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. S2CID 18759600.catalog entry
- Torres, C. A. O.; et al. (December 2006). "Search for associations containing young stars (SACY). I. Sample and searching method". Astronomy and Astrophysics. 460 (3): 695–708. arXiv:astro-ph/0609258. Bibcode:2006A&A...460..695T. doi:10.1051/0004-6361:20065602. S2CID 16080025.
- 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.
- Johnson, H. L.; et al. (1966), "UBVRIJKL photometry of the bright stars", Communications of the Lunar and Planetary Laboratory, 4 (99), Bibcode:1966CoLPL...4...99J
- 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.
- Allende Prieto, C.; Lambert, D. L. (December 1999). "Fundamental parameters of nearby stars from the comparison with evolutionary calculations: masses, radii and effective temperatures". Astronomy and Astrophysics. 352: 555–562. arXiv:astro-ph/9911002. Bibcode:1999A&A...352..555A. ISSN 0004-6361.
- 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.