HR 6806

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Template:Short description

HR 6806
Observation data
Epoch J2000      Equinox J2000
Constellation Hercules[1]
Right ascension Template:RA[2]
Declination Template:DEC[2]
Apparent magnitude (V) 6.40[3]
Characteristics
Spectral type K2 V[4]
U−B Template:Engvar +0.585[3]
B−V Template:Engvar +0.875[3]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[2] km/s
Proper motion (μ) RA: −316.520[2] mas/yr
Dec.: −468.214[2] mas/yr
Parallax (π)90.1264±0.0200 mas[2]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)6.17[5]
Details
MassScript error: No such module "val".[6] Template:Solar mass
RadiusScript error: No such module "val".[6] Template:Solar radius
Luminosity0.35[6] Template:Solar luminosity
Surface gravity (log g)4.53[4] cgs
Temperature4,900[4] K
Metallicity [Fe/H]−0.61[4] dex
Rotation42 d[7]
Rotational velocity (v sin i)4.82[8] km/s
Age5.8–7.1[9] Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[10]
Database references
SIMBADdata

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HR 6806 or HD 166620 is a solitary, orange, main sequence, and Sun-like (K2 V) star located thirty-six light-years away,[11] in the constellation Hercules. The star is smaller than the Sun, with around 79% of the solar mass and radius, and 35% of the solar luminosity.[6] It appears to be rotating slowly with an estimated period of 42 days. In 1988, it was noticed that the star had an inactive chromosphere, with a surface magnetic field strength of only 1,500 G.[7] From 1990 activity in the chromosphere increased, inline with a 16 year stellar cycle previously observed. But, sometime after 1994 (exact date unknown because of a data collection gap between 1995 and 2004) chromospheric activity greatly reduced, and has stayed flat for more than 16 years. As of 2022,Template:Dated maintenance category (articles)Script error: No such module "Check for unknown parameters". the star appears to have entered the equivalent of a Maunder minimum.[11] The star is around six billion years of age.[9]

There was suspected to be a nearby very cool, and very dim, T9 to Y brown dwarf companion, WISE J180901.07+383805.4, at an angular separation of 769″, which would have corresponded to a projected separation of 8460 AU at the distance of HR 6806. However, with further observation it was found to be bluer than at first thought and more typical of a slightly brighter T7 dwarf, which would place it at a much greater distance of Script error: No such module "convert".—ruling out a physical association. This is confirmed by the differing proper motion of the star and this object.[12]

References

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External links

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  • NStars: 1809+3827Script error: No such module "Unsubst".

Template:Stars of Hercules