HD 19789
This article will address the issue of HD 19789, which has become a topic of great relevance today. For some years now, HD 19789 has aroused great interest in different areas, being the subject of debate, analysis and reflection by experts and scholars. Its influence and impact on today's society has led to numerous studies, research and projects being dedicated to it in various fields, seeking to understand its multiple facets and effects. Therefore, this article aims to explore and delve into the different dimensions that surround HD 19789, in order to offer a broad and complete vision of this topic that is so relevant today.
| Observation data Epoch J2000.0 Equinox J2000.0 | |
|---|---|
| Constellation | Aries[1] |
| Right ascension | 03h 11m 21.91898s[2] |
| Declination | +13° 02′ 52.2342″[2] |
| Apparent magnitude (V) | 6.11[1] |
| Characteristics | |
| Evolutionary stage | red giant branch[2] |
| Spectral type | K0IIIp[3] |
| B−V color index | 1.038±0.012[1] |
| Astrometry | |
| Radial velocity (Rv) | +8.10±0.32[1] km/s |
| Proper motion (μ) | RA: −15.387[2] mas/yr Dec.: +16.445[2] mas/yr |
| Parallax (π) | 8.4809±0.0283 mas[2] |
| Distance | 385 ± 1 ly (117.9 ± 0.4 pc) |
| Absolute magnitude (MV) | 0.53[1] |
| Details | |
| Mass | 2.6[2] M☉ |
| Radius | 11[2] R☉ |
| Luminosity | 63[2] L☉ |
| Surface gravity (log g) | 2.67[2] cgs |
| Temperature | 4.933[2] K |
| Age | 558[2] Myr |
| 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.[1] it is located at a distance of approximately 385 light years from the Sun based on parallax,[2] and is drifting further away with a radial velocity of +8 km/s.[1] 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 63 times the Sun's luminosity from its swollen photosphere at an effective temperature of 4,933 K.[2] 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 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. XHIP record for this object at VizieR.
- ^ a b c d e f g h i j k l m n Vallenari, A.; et al. (Gaia collaboration) (2023). "Gaia Data Release 3. Summary of the content and survey properties". Astronomy and Astrophysics. 674: A1. arXiv:2208.00211. Bibcode:2023A&A...674A...1G. doi:10.1051/0004-6361/202243940. S2CID 244398875. Gaia DR3 record for this source at VizieR.
- ^ 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
