HD 196050

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HD 196050
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
Distance165.5 ± 0.3 ly
(50.7 ± 0.1 pc)
Absolute magnitude (MV)4.01[2]
Details[5]
A
Mass1.18±0.02[1] M☉
Radius1.46+0.02
−0.03 R☉
Luminosity2.213+0.007
−0.006[1] L☉
Surface gravity (log g)4.32 cgs
Temperature5,834+55
−52[1] K
Metallicity [Fe/H]0.34±0.06 dex
Rotation16.0 d[6]
Rotational velocity (v sin i)3.0 km/s
Age2.5±1.3 Gyr
Other designations
CPD−61° 6497, HD 196050, HIP 101806, SAO 254837, PPM 364690, WDS J20379-6038AB[7]
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia		data

HD 196050 is a triple star[8][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.

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.[8] 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,[8] located 10.80″[3] to the south of the primary component. This corresponds to a projected separation of 7,511±22 AU.[8] The star is magnitude 10.62[3] A third companion, component C, was discovered in 2007, located about 0.4″ from component B.[9] 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.[10] The discovery was independently confirmed by the Geneva Extrasolar Planet Search team.[6]

The HD 196050 planetary system[11]
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 — —

See also[]

References[]

  1. ^ a b c d e f g h i j k 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.
  2. ^ 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. S2CID 119257644.
  3. ^ a b c d e f g 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
  4. ^ a b Houk, Nancy (1979). Michigan catalogue of two-dimensional spectral types for the HD stars. Vol. 1. Ann Arbor, Michigan: Department of Astronomy, University of Michigan. Bibcode:1978mcts.book.....H.
  5. ^ a b 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): 3162–3177. arXiv:1905.12066. Bibcode:2019MNRAS.487.3162C. doi:10.1093/mnras/stz1496. S2CID 168169634.
  6. ^ a b 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. S2CID 5233877.
  7. ^ "HD 196050". SIMBAD. Centre de données astronomiques de Strasbourg. Retrieved 2018-07-25.
  8. ^ a b c d 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. S2CID 14065040.
  9. ^ 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. S2CID 55755453. A92.
  10. ^ Jones, Hugh R. A.; et al. (December 2002). "Extrasolar planets around HD 196050, HD 216437 and HD 160691". Monthly Notices 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. S2CID 119520409.
  11. ^ 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. S2CID 119067572.

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.

Coordinates: Sky map 20h 37m 51.7098s, −60° 38′ 04.147″

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