Astronomy:HD 111456
| Observation data Equinox J2000.0]] (ICRS) | |
|---|---|
| Constellation | Ursa Major[1] |
| Right ascension | 12h 48m 39.44700s[2] |
| Declination | 60° 19′ 11.0379″[2] |
| Apparent magnitude (V) | 5.85[3] |
| Characteristics | |
| Evolutionary stage | main sequence[4] |
| Spectral type | F7 V[5] |
| U−B color index | −0.04[3] |
| B−V color index | +0.46[3] |
| Astrometry | |
| Radial velocity (Rv) | −18.0±0.9[6] km/s |
| Proper motion (μ) | RA: +120.949[2] mas/yr Dec.: +35.712[2] mas/yr |
| Parallax (π) | 38.1905 ± 0.2904[2] mas |
| Distance | 85.4 ± 0.6 ly (26.2 ± 0.2 pc) |
| Absolute magnitude (MV) | +4.2±0.2[4] |
| Details | |
| Mass | 1.4[7] M☉ |
| Radius | 1.22[4] R☉ |
| Luminosity | 6.45[1] L☉ |
| Surface gravity (log g) | 4.5[4] cgs |
| Temperature | 6,400[4] K |
| Metallicity [Fe/H] | −0.19[8] dex |
| Rotation | 14.7[9] days |
| Rotational velocity (v sin i) | 41.5±1.1[4] km/s |
| Age | 300−400[4] Myr |
| Other designations | |
| Database references | |
| SIMBAD | data |
HD 111456 is a yellow-white hued star in the northern circumpolar constellation of Ursa Major. It is dimly visible to the naked eye, having an apparent visual magnitude of 5.85.[3] Based upon an annual parallax shift of 38.2 mas as seen from Earth, it is located about 85 light years from the Sun. The star is moving closer to the Sun with a radial velocity of −18 km/s.[6] HD 111456 is a nucleus cluster member of the Ursa Major Moving Group, a set of stars that are moving through space with a similar heading and velocity. Six other stars in the nucleus of the group are prominent members of the Big Dipper asterism.[5]
The stellar classification for this star is F7 V,[5] indicating that it is an ordinary F-type main-sequence star. It is young, around 300−400 million years of age, and is spinning with a relatively high projected rotational velocity of 41.5 km/s.[4] This is one of the most active F-type stars known, and it is a strong emitter of X-rays[4] and an extreme UV source. It is an astrometric binary with a period of four years and a mass ratio of 0.5. Hence, the companion may be a young white dwarf star.[11]
References
- ↑ 1.0 1.1 Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters 38 (5): 331, doi:10.1134/S1063773712050015, Bibcode: 2012AstL...38..331A.
- ↑ 2.0 2.1 2.2 2.3 2.4 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.
- ↑ 3.0 3.1 3.2 3.3 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.
- ↑ 4.0 4.1 4.2 4.3 4.4 4.5 4.6 4.7 4.8 Freire Ferrero, R. et al. (January 2004), "Magnetic activity in HD 111456, a young F5-6 main-sequence star", Astronomy and Astrophysics 413 (2): 657−667, doi:10.1051/0004-6361:20031565, Bibcode: 2004A&A...413..657F.
- ↑ 5.0 5.1 5.2 Levato, H.; Abt, H. A. (August 1978), "Spectral types in the Ursa Major stream", Publications of the Astronomical Society of the Pacific 90: 429−433, doi:10.1086/130352, Bibcode: 1978PASP...90..429L.
- ↑ 6.0 6.1 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.
- ↑ Reiners, Ansgar; Zechmeister, Mathias (2020), "Radial Velocity Photon Limits for the Dwarf Stars of Spectral Classes F-M", The Astrophysical Journal Supplement Series 247 (1): 11, doi:10.3847/1538-4365/ab609f, Bibcode: 2020ApJS..247...11R.
- ↑ Netopil, Martin (2017), "Metallicity calibrations for dwarf stars and giants in the Geneva photometric system", Monthly Notices of the Royal Astronomical Society 469 (3): 3042, doi:10.1093/mnras/stx1077, Bibcode: 2017MNRAS.469.3042N.
- ↑ Colman, Isabel L.; Angus, Ruth; David, Trevor; Curtis, Jason; Hattori, Soichiro; Lu, Yuxi (Lucy) (2024), "Methods for the Detection of Stellar Rotation Periods in Individual TESS Sectors and Results from the Prime Mission", The Astronomical Journal 167 (5): 189, doi:10.3847/1538-3881/ad2c86, Bibcode: 2024AJ....167..189C.
- ↑ "HR 4867". SIMBAD. Centre de données astronomiques de Strasbourg. http://simbad.u-strasbg.fr/simbad/sim-basic?Ident=HR+4867.
- ↑ Goldin, A.; Makarov, V. V. (September 2006), "Unconstrained Astrometric Orbits for Hipparcos Stars with Stochastic Solutions", The Astrophysical Journal Supplement Series 166 (1): 341−350, doi:10.1086/505939, Bibcode: 2006ApJS..166..341G.
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