HD 196885

Last updated
HD 196885
Observation data
Epoch J2000       Equinox J2000
Constellation Delphinus
Right ascension 20h 39m 51.87531s [1]
Declination +11° 14′ 58.7029″ [1]
Apparent magnitude  (V)6.39 [2]
Characteristics
Evolutionary stage main-sequence star
Spectral type F8V [3] + M1±1V [4]
B−V color index 0.559±0.006 [2]
Astrometry
Radial velocity (Rv)−30.13±0.09 [2]  km/s
Proper motion (μ)RA: +71.470±0.066 [1]   mas/yr
Dec.: +89.165±0.076 [1]   mas/yr
Parallax (π)29.4076 ± 0.0272  mas [5]
Distance 110.9 ± 0.1  ly
(34.00 ± 0.03  pc)
Absolute magnitude  (MV)3.76 [2]
Orbit [6]
PrimaryHD 196885 A
CompanionHD 196886 B
Period (P)69.045 yr
Semi-major axis (a)19.778 AU
Eccentricity (e)69.045
Inclination (i)120.427°
Longitude of the node (Ω)79.150°
Periastron epoch (T)1982.886 AD
Argument of periastron (ω)
(secondary)		231.464°
Details [6]
A
Mass 1.33  M☉
Radius 1.45+0.02
−0.05  R☉
Luminosity 2.695±0.006 [1]   L☉
Surface gravity (log g)4.46±0.02  cgs
Temperature 6,340±39  K
Metallicity [Fe/H]0.29±0.05  dex
Rotation 15 days
Rotational velocity (v sin i)7.3±1.5 km/s
Age 2.0±0.5  Gyr
B
Mass 0.508±0.001 [6]   M☉
Other designations
BD+10° 4351, GC  28784, HD  196885, HIP  101966, HR  7907, SAO  106360, WDS J20399+1115, GCRV  12946, GSC  01092-01778, 2MASS J20395188+1114588 [7]
Database references
SIMBAD data

HD 196885 is a binary star system in the northern constellation of Delphinus. It comprise a pair of stars HD 196885 A and HD 196885 B on a 69-years eccentric orbit. [6]

Contents

The primary star is near the lower limit of visibility to the naked eye with an apparent visual magnitude of 6.39. [2] It is located at a distance of 110.9  light years from the Sun. [5] It is drifting closer with a radial velocity of −30 km/s, and is expected to come to within 52.5 light-years in 836,000 years. [2]

The secondary, component B, is a red dwarf star separated by 0.6 arcseconds from the primary star that was discovered in 2006 with NaCo at VLT. [8] [4] It has a class in the range M1V to M3V [4] with 51% of the Sun's mass. [6]

The star BD+10 4351B, located 192 arcseconds away from HD 196885 is located at the same distance and may be a physically bound companion star, in which case HD 196885 is a triple system. [9] If it is bound, then the separation is at least 6,600 AU (the separation along the line-of-sight is unknown, so this value represents a lower limit on the true separation).[ citation needed ]

Planetary system

In 2004, a planet was announced to be orbiting the star HD 196885 A in a 386-day orbit. [10] Follow-up work published in 2008 did not confirm the original candidate but instead found evidence of a planet in a 3.63 years. [11] Perturbation by the secondary star in this system may have driven the planet into a high inclination orbit. [12] The planetary existence was confirmed and parameters were refined by 2022. [6]

The HD 196885 planetary system [6]
Companion
(in order from star)		 Mass Semimajor axis
(AU)		 Orbital period
(years)		 Eccentricity Inclination Radius
b 3.39  MJ 2.3833.4850.444143.041° —

See also

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References

  1. 1 2 3 4 5 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. 1 2 3 4 5 6 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. ↑ Gray, R. O.; et al. (2001), "The Physical Basis of Luminosity Classification in the Late A-, F-, and Early G-Type Stars. I. Precise Spectral Types for 372 Stars", The Astronomical Journal, 121 (4): 2148, Bibcode:2001AJ....121.2148G, doi:10.1086/319956, S2CID   117076031
  4. 1 2 3 Chauvin, G.; et al. (2007). "Characterization of the long-period companions of the exoplanet host stars: HD 196885, HD 1237 and HD 27442". Astronomy and Astrophysics. 475 (2): 723–727. arXiv: 0710.5918 . Bibcode:2007A&A...475..723C. doi:10.1051/0004-6361:20067046. S2CID   16950822.
  5. 1 2 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 .
  6. 1 2 3 4 5 6 7 Chauvin, G.; Videla, M.; Beust, H.; Mendez, R.; Correia, A. C. M.; Lacour, S.; Tokovinin, A.; Hagelberg, J.; Bouchy, F.; Boisse, I.; Villegas, C.; Bonavita, M.; Desidera, S.; Faramaz, V.; Forveille, T.; Gallenne, A.; Haubois, X.; Jenkins, J. S.; Kervella, P.; Lagrange, A. -M.; Melo, C.; Thebault, P.; Udry, S.; Segransan, D. (2023), "Chasing extreme planetary architectures", Astronomy & Astrophysics, 675: A114, arXiv: 2211.00994 , doi:10.1051/0004-6361/202244502
  7. ↑ "HD 196885". SIMBAD . Centre de données astronomiques de Strasbourg . Retrieved 2020-08-08.
  8. ↑ Chauvin, G.; et al. (2006). "Probing long-period companions to planetary hosts. VLT and CFHT near infrared coronographic imaging surveys". Astronomy and Astrophysics. 456 (3): 1165–1172. arXiv: astro-ph/0606166 . Bibcode:2006A&A...456.1165C. doi:10.1051/0004-6361:20054709. S2CID   15611548.
  9. ↑ "HD 196885 A page". Geneva Observatory . Retrieved 2008-08-19.
  10. ↑ "The Planet Around HD 196885". California & Carnegie Planet Search Team (Internet Archive link). Archived from the original on 2004-12-27. Retrieved 2008-08-19.
  11. ↑ Correia, A. C. M.; et al. (2008). "The ELODIE survey for northern extra-solar planets. IV. HD 196885, a close binary star with a 3.7-year planet". Astronomy and Astrophysics . 479 (1): 271–275. arXiv: 0711.3343 . Bibcode:2008A&A...479..271C. doi:10.1051/0004-6361:20078908. S2CID   119261807.
  12. ↑ Satyal, S.; Hinse, T. C.; Quarles, B.; Noyola, J. P. (September 2014). "Chaotic dynamics of the planet in HD 196885 AB". Monthly Notices of the Royal Astronomical Society. 443 (2): 1310–1318. arXiv: 1401.1268 . Bibcode:2014MNRAS.443.1310S. doi:10.1093/mnras/stu1221. S2CID   119189415.
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