HD 195564
| Observation data Epoch J2000.0 Equinox ICRS | |
|---|---|
| Constellation | Capricornus[1] |
| Right ascension | 20h 32m 23.695s[2] |
| Declination | −09° 51′ 12.18″[2] |
| Apparent magnitude (V) | 5.65[3] |
| Characteristics | |
| Evolutionary stage | subgiant[2] |
| Spectral type | G2.5IV[4] |
| U−B color index | +0.20[3] |
| B−V color index | +0.68[3] |
| Astrometry | |
| Radial velocity (Rv) | +9.58[5] km/s |
| Proper motion (μ) | RA: +309.736 mas/yr[2] Dec.: +109.910 mas/yr[2] |
| Parallax (π) | 40.4241±0.0497 mas[2] |
| Distance | 80.68 ± 0.10 ly (24.74 ± 0.03 pc) |
| Absolute magnitude (MV) | +3.72[1] |
| Orbit[6] | |
| Primary | 620+300 −170 years |
| Semi-major axis (a) | 88+26 −17 au |
| Eccentricity (e) | 0.917+0.037 −0.064 |
| Inclination (i) | 64.3+5.7 −6.0° |
| Details | |
| HD 195564 A | |
| Mass | 1.242+0.062 −0.060[6] M☉ |
| Radius | 1.894±0.080[7] R☉ |
| Luminosity | 2.986±0.018[7] L☉ |
| Surface gravity (log g) | 3.95±0.05[7] cgs |
| Temperature | 5,514±116[7] K |
| Metallicity [Fe/H] | 0.05±0.02[7] dex |
| Rotational velocity (v sin i) | 1.91[8] km/s |
| Age | 8.2[9] Gyr |
| HD 195564 B | |
| Mass | 0.520+0.027 −0.026[6] M☉ |
| Other designations | |
| BD−10°5423, FK5 1536, GJ 792.1, HD 195564, HIP 101345, HR 7845, SAO 163665[10] | |
| Database references | |
| SIMBAD | data |
| ARICNS | data |
HD 195564 is a binary star in the southern constellation of Capricornus. It is faintly visible to the naked eye with an apparent visual magnitude of 5.65.[3] Parallax measurements give us an estimate of its distance as 81 light years.
Based upon the spectrum of light emitted by the primary, it has a stellar classification of G2.5IV.[4] This indicates that it is a G-type subgiant that has exhausted the hydrogen in its core region. It has a mass of 1.242 times the mass of the Sun,[6] but a measured radius that is 1.894 times as large.[7] As a result, it shines with 2.986 times the luminosity of the Sun.[7] The abundance of elements in this star is similar to that in the Sun, although it is an older star with an age of around 8.2 billion years.[9] The effective temperature of the stellar atmosphere is 5,514 K,[7] giving it the yellow-hued glow of an ordinary K-type star.[11]
The secondary companion has an apparent magnitude of 11.30,[12] and a mass just 55% that of the Sun.[13] The pair orbit each other with an estimated period of around 620 years, following a highly-eccentric path.[6]
In a paper published in April 2017, a candidate planet was found orbiting HD 195564 A with a period of 5,404 days (14.80 yr).[14]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination (°) |
Radius |
|---|---|---|---|---|---|---|
| b (unconfirmed) | — | — | 5403±164 | — | — | — |
References
- 1 2 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.
- 1 2 3 4 5 6 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.
- 1 2 3 4 Mermilliod, J.-C. (1986), "Compilation of Eggen's UBV data, transformed to UBV (unpublished)", Catalogue of Eggen's UBV Data, SIMBAD, Bibcode:1986EgUBV........0M.
- 1 2 Keenan, Philip C.; McNeil, Raymond C. (1989). "The Perkins Catalog of Revised MK Types for the Cooler Stars". The Astrophysical Journal Supplement Series. 71: 245. Bibcode:1989ApJS...71..245K. doi:10.1086/191373.
- ↑ Nidever, David L.; et al. (August 2002), "Radial Velocities for 889 Late-Type Stars", The Astrophysical Journal Supplement Series, 141 (2): 503–522, arXiv:astro-ph/0112477, Bibcode:2002ApJS..141..503N, doi:10.1086/340570, S2CID 51814894.
- 1 2 3 4 5 An, Qier; Brandt, Timothy D.; Brandt, G. Mirek; Venner, Alexander (October 2025), "Orbits and Masses for 156 Companions from Combined Astrometry and Radial Velocities, and a Validation of Gaia Non-single-star Solutions", The Astrophysical Journal Supplement Series, 280 (2): 61, arXiv:2508.08374, Bibcode:2025ApJS..280...61A, doi:10.3847/1538-4365/adfa99, ISSN 0067-0049.
- 1 2 3 4 5 6 7 8 Soubiran, C.; Creevey, O. L.; Lagarde, N.; Brouillet, N.; Jofré, P.; Casamiquela, L.; Heiter, U.; Aguilera-Gómez, C.; Vitali, S.; Worley, C.; de Brito Silva, D. (2024-02-01). "Gaia FGK benchmark stars: Fundamental Teff and log g of the third version". Astronomy and Astrophysics. 682: A145. arXiv:2310.11302. Bibcode:2024A&A...682A.145S. doi:10.1051/0004-6361/202347136. ISSN 0004-6361. S2CID 264172605.
- ↑ Martínez-Arnáiz, R.; et al. (September 2010), "Chromospheric activity and rotation of FGK stars in the solar vicinity. An estimation of the radial velocity jitter", Astronomy and Astrophysics, 520: A79, arXiv:1002.4391, Bibcode:2010A&A...520A..79M, doi:10.1051/0004-6361/200913725, S2CID 43455849.
- 1 2 Boyajian, Tabetha S.; et al. (July 2013), "Stellar Diameters and Temperatures. III. Main-sequence A, F, G, and K Stars: Additional High-precision Measurements and Empirical Relations", The Astrophysical Journal, 771 (1): 31, arXiv:1306.2974, Bibcode:2013ApJ...771...40B, doi:10.1088/0004-637X/771/1/40, S2CID 14911430, 40. See Table 3.
- ↑ "HD 195564". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved March 15, 2016.
- ↑ "The Colour of Stars", Australia Telescope, Outreach and Education, Commonwealth Scientific and Industrial Research Organisation, December 21, 2004, archived from the original on March 18, 2012, retrieved 2012-01-16.
- ↑ Mason, B. D.; et al. (2014), "The Washington Visual Double Star Catalog", The Astronomical Journal, 122 (6): 3466–3471, Bibcode:2001AJ....122.3466M, doi:10.1086/323920, retrieved 2015-07-22.
- ↑ Tokovinin, Andrei (April 2014), "From Binaries to Multiples. II. Hierarchical Multiplicity of F and G Dwarfs", The Astronomical Journal, 147 (4): 14, arXiv:1401.6827, Bibcode:2014AJ....147...87T, doi:10.1088/0004-6256/147/4/87, S2CID 56066740, 87.
- 1 2 Butler, R. Paul; et al. (13 April 2017). "The LCES HIRES/Keck Precision Radial Velocity Exoplanet Survey". The Astronomical Journal. 153 (5): 208. arXiv:1702.03571. Bibcode:2017AJ....153..208B. doi:10.3847/1538-3881/aa66ca. hdl:2299/18220. S2CID 14954371. Planet candidate is in Table 2; full table available here.
- Gray, R. O.; et al. (2003), "Contributions to the Nearby Stars (NStars) Project: Spectroscopy of Stars Earlier than M0 within 40 Parsecs: The Northern Sample. I", The Astronomical Journal, 126 (4): 2048–2059, arXiv:astro-ph/0308182, Bibcode:2003AJ....126.2048G, doi:10.1086/378365, S2CID 119417105.
