HD 196885

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Template:Short description

HD 196885
Observation data
Epoch J2000      Equinox J2000
Constellation Delphinus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 6.39[2]
Characteristics
Evolutionary stage main-sequence star
Spectral type F8V[3] + M1±1V[4]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: Script error: No such module "val".[1] mas/yr
Dec.: Script error: No such module "val".[1] mas/yr
Parallax (π)29.4076±0.0272 mas[5]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.76[2]
Orbit[6]
PrimaryHD 196885 A
CompanionHD 196886 B
Period (P)72.06 ± 4.59 yr
Semi-major axis (a)21.00 ± 0.86 AU
Eccentricity (e)0.42 ± 0.03
Inclination (i)116.8 ± 0.7°
Longitude of the node (Ω)79.150°
Periastron epoch (T)1982.886 AD
Argument of periastron (ω)
(secondary)
231.464°
Details[6]
A
Mass1.3 ± 0.1 Template:Solar mass
RadiusScript error: No such module "val".Script error: No such module "Unsubst". Template:Solar radius
LuminosityScript error: No such module "val".[1] Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]Script error: No such module "val". dex
Rotation15 daysScript error: No such module "Unsubst".
Rotational velocity (v sin i)Script error: No such module "val".Script error: No such module "Unsubst". km/s
Age1.5—3.5 Gyr
B
MassScript error: No such module "val".[6] Template:Solar mass
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[7]
Database references
SIMBADdata

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

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 Script error: No such module "convert". 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 trinary 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).Script error: No such module "Unsubst".

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 Script error: No such module "convert"..[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]

Template:OrbitboxPlanet begin Template:OrbitboxPlanet

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See also

References

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Template:Sky Template:Stars of Delphinus