HD 196050
HD 196050 is a triple star[7][3] system located in the southern constellation of Pavo. This system has an apparent magnitude of 7.50[2] and the absolute magnitude is 4.01.[2] It is located at a distance of 112 light years from the Sun based on parallax, and is drifting further away with a radial velocity of +61 km/s.[2] It is also called by the Hipparcos number 101806.
| Observation data Epoch J2000 Equinox J2000 | |
|---|---|
| Constellation | Pavo |
| Right ascension | 20h 37m 51.70984s[1] |
| Declination | −60° 38′ 04.1473″[1] |
| Apparent magnitude (V) | 7.50[2] + 10.62[3] + 15.6[3] |
| Characteristics | |
| Spectral type | G3V[4] + M1.5-M4.5 + M2.5-M5.5[3] |
| B−V color index | 0.667±0.010[2] |
| Astrometry | |
| Radial velocity (Rv) | +61.37±0.14[2] km/s |
| Proper motion (μ) | RA: −191.122±0.061[1] mas/yr Dec.: −64.922±0.054[1] mas/yr |
| Parallax (π) | 19.7051 ± 0.0394[1] mas |
| Distance | 165.5 ± 0.3 ly (50.7 ± 0.1 pc) |
| Absolute magnitude (MV) | 4.01[2] |
| Details[5] | |
| A | |
| Mass | 1.18±0.02[1] M☉ |
| Radius | 1.46+0.02 −0.03 R☉ |
| Luminosity | 2.213+0.007 −0.006[1] L☉ |
| Surface gravity (log g) | 4.32 cgs |
| Temperature | 5,834+55 −52[1] K |
| Metallicity [Fe/H] | 0.34±0.06 dex |
| Rotational velocity (v sin i) | 3.0 km/s |
| Age | 2.5±1.3 Gyr |
| Other designations | |
| Database references | |
| SIMBAD | data |
| Extrasolar Planets Encyclopaedia | data |
The primary component is a G-type main-sequence star with a stellar classification of G3V.[4] It has a quiescent chromosphere and does not appear to be variable.[7] The star has 18%[1] more mass than the Sun and a 46% greater size. It is around 2.5 billion years old with a higher than solar metallicity, and is spinning with a projected rotational velocity of 3 km/s.[5] The star is radiating 2.21[1] times the luminosity of the Sun from its photosphere at an effective temperature of 5.834 K.[1]
A faint co-moving companion star, designated component B, was detected based on observations during 2003–2004,[7] located 10.80″[3] to the south of the primary component. This corresponds to a projected separation of 7,511±22 AU.[7] The star is magnitude 10.62[3] A third companion, component C, was discovered in 2007, located about 0.4″ from component B.[8] It has a visual magnitude of 15.6.[3]
In 2002, the Anglo-Australian Planet Search team announced the discovery of an extrasolar planet orbiting the star.[9] The discovery was independently confirmed by the Geneva Extrasolar Planet Search team.[10]
| Companion (in order from star) |
Mass | Semimajor axis (AU) |
Orbital period (days) |
Eccentricity | Inclination | Radius |
|---|---|---|---|---|---|---|
| b | ≥2.90±0.26 MJ | 2.54±0.15 | 1,378±21 | 0.228±0.038 | — | — |
References
- 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.
- 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.
- Mason, B. D.; et al. (2014), The Washington Visual Double Star Catalog, Bibcode:2001AJ....122.3466M, doi:10.1086/323920, retrieved 2015-07-22
- Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. 1. Ann Arbor, Michigan: Department of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
- Chavero, C.; et al. (August 2019). "Emerging trends in metallicity and lithium properties of debris disc stars". Monthly Notices of the Royal Astronomical Society. 487 (3, p.3162-3177). arXiv:1905.12066. Bibcode:2019MNRAS.487.3162C. doi:10.1093/mnras/stz1496.
- "HD 196050". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-25.
- Mugrauer, M.; et al. (2005). "Four new wide binaries among exoplanet host stars". Astronomy and Astrophysics. 440 (3): 1051–1060. arXiv:astro-ph/0507101. Bibcode:2005A&A...440.1051M. doi:10.1051/0004-6361:20042297.
- Roell, T.; et al. (June 2012). "Extrasolar planets in stellar multiple systems". Astronomy & Astrophysics. 542: 10. arXiv:1204.4833. Bibcode:2012A&A...542A..92R. doi:10.1051/0004-6361/201118051. A92.
- Jones, Hugh R. A.; et al. (December 2002). "Extrasolar planets around HD 196050, HD 216437 and HD 160691". Monthly Notice of the Royal Astronomical Society. 337 (4): 1170–1178. arXiv:astro-ph/0206216. Bibcode:2002MNRAS.337.1170J. doi:10.1046/j.1365-8711.2002.05787.x.
- Mayor, M.; et al. (2004). "The CORALIE survey for southern extra-solar planets XII. Orbital solutions for 16 extra-solar planets discovered with CORALIE". Astronomy and Astrophysics. 415 (1): 391–402. arXiv:astro-ph/0310316. Bibcode:2004A&A...415..391M. doi:10.1051/0004-6361:20034250.
- Butler, R. P.; et al. (2006). "Catalog of Nearby Exoplanets". The Astrophysical Journal. 646 (1): 505–522. arXiv:astro-ph/0607493. Bibcode:2006ApJ...646..505B. doi:10.1086/504701.
Further reading
- Greenhill, L.; et al. (2002). "epsilon Eridani, upsilon Andromedae, 51 Pegasi, HD 209458, HD 196050". IAU Circular. 7985: 1. Bibcode:2002IAUC.7985....1G.