HD 19789
The topic of HD 19789 is one of the most relevant today. With an impact that spans all aspects of society, HD 19789 has captured the attention of experts and everyday people alike. Since its emergence, HD 19789 has generated debates, controversies and has been the subject of numerous investigations and studies. The importance of understanding and analyzing HD 19789 lies in its influence in various areas, including economics, politics, health, technology and the environment. In this article, we will thoroughly explore the dimensions and impacts of HD 19789, as well as possible strategies to address its challenges.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Aries |
| Right ascension | 03h 11m 21.91887s[1] |
| Declination | +13° 02′ 52.2356″[1] |
| Apparent magnitude (V) | 6.11[2] |
| Characteristics | |
| Spectral type | K0IIIp[3] |
| B−V color index | 1.038±0.012[2] |
| Astrometry | |
| Radial velocity (Rv) | +8.10±0.32[2] km/s |
| Proper motion (μ) | RA: −15.291[1] mas/yr Dec.: +16.363[1] mas/yr |
| Parallax (π) | 8.3619±0.0857 mas[1] |
| Distance | 390 ± 4 ly (120 ± 1 pc) |
| Absolute magnitude (MV) | 0.53[2] |
| Details | |
| Radius | 10.95+0.34 −0.25[1] R☉ |
| Luminosity | 58.5±0.7[1] L☉ |
| Temperature | 4,822+57 −72[1] K |
| Other designations | |
| BD+12°452, FK5 2488, HD 19789, HIP 14821, HR 952, SAO 93327, WDS WDS J03114+1303AB[4] | |
| Database references | |
| SIMBAD | data |
HD 19789 is a double star in the northern constellation of Aries. The primary component has an orange hue and is barely visible to the naked eye with an apparent visual magnitude of 6.11.[2] it is located at a distance of approximately 390 light years from the Sun based on parallax,[1] and is drifting further away with a radial velocity of +8 km/s.[2] The star is located near the ecliptic and thus is subject to lunar occultations.[5]
The primary, designated component A, is an aging giant star with a stellar classification of K0IIIp,[3] where the 'p' suffix indicates some type of unspecified peculiarity in the spectrum. It has exhausted the supply of hydrogen at its core, then expanded and cooled off the main sequence: at present it has 11 times the girth of the Sun. The star is radiating 58.5 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4822 K.[1] It has one reported companion, component B, at an angular separation of 0.5″ along a position angle of 23°, as of 1982.[6]
References
- ^ a b c d e f g h i j 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.
- ^ a b c d e f Anderson, E.; Francis, Ch. (2012), "XHIP: An extended hipparcos compilation", Astronomy Letters, 38 (5): 331, arXiv:1108.4971, Bibcode:2012AstL...38..331A, doi:10.1134/S1063773712050015, S2CID 119257644.
- ^ a b Harlan, E. A. (September 1969), "MK classifications for F- and G-type stars. I", Astronomical Journal, 74: 916–919, Bibcode:1969AJ.....74..916H, doi:10.1086/110881.
- ^ "HD 19789". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2011-12-20.
- ^ Blow, G. L.; et al. (November 1982), "Photoelectric observations of lunar occultations. XIII", Astronomical Journal, 87: 1571–1584, Bibcode:1982AJ.....87.1571B, doi:10.1086/113247. See entry 5931, p. 1580, SAO 93327.
- ^ 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, retrieved 2015-07-22
