HD 205739

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HD 205739 / Sāmaya
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Piscis Austrinus
Right ascension Template:RA[1]
Declination Template:DEC[1]
Apparent magnitude (V) 8.56[2]
Characteristics
Spectral type F7 V[3]
B−V Template:Engvar Script error: No such module "val".[2]
Astrometry
Radial velocity (Rv)Script error: No such module "val".[1] km/s
Proper motion (μ) RA: +21.833 mas/yr[1]
Dec.: −82.314 mas/yr[1]
Parallax (π)10.7609±0.0203 mas[1]
DistanceTemplate:Rnd ± Template:Rnd ly
(Template:Rnd ± Template:Rnd pc)
Absolute magnitude (MV)3.42[2]
Details[4]
MassScript error: No such module "val". Template:Solar mass
RadiusScript error: No such module "val". Template:Solar radius
LuminosityScript error: No such module "val". Template:Solar luminosity
Surface gravity (log g)Script error: No such module "val". cgs
TemperatureScript error: No such module "val". K
Metallicity [Fe/H]0.21[5] dex
Rotational velocity (v sin i)4.06[5] km/s
AgeScript error: No such module "val". Gyr
Metallicity [Fe/H]{{{metal_fe2}}} dex
Other designations
Template:Odlist[6]
Database references
SIMBADdata
Exoplanet Archivedata

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HD 205739 is a yellow-white hued star in the southern constellation of Piscis Austrinus, positioned near the western constellation boundary with Microscopium. It has the proper name Sāmaya, which was selected in the NameExoWorlds campaign by Sri Lanka, during the 100th anniversary of the IAU. Sāmaya (

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Template:Redirect template) means peace in the Sinhalese language.[7][8]

With an apparent visual magnitude of 8.56,[2] this star requires a small telescope to view. It is located at a distance of approximately 303 light-years from the Sun based on stellar parallax, and is drifting further away with a radial velocity of +9.7 km/s.[1] This star has an absolute magnitude of 3.42.[2]

HD 205739 is an ordinary F-type main-sequence star with a stellar classification of F7 V.[3] This indicates that, like the Sun, it is generating energy through core hydrogen fusion. The star is 2.8[4] billion years old with an inactive chromosphere[9] and is spinning with a projected rotational velocity of 4 km/s.[5] It has 1.3 times the mass of the Sun and 1.6 times the Sun's radius.[4] The abundance of iron is 60% greater than in the Sun, suggesting a higher metallicity.[5] The star is radiating 3.5 times the luminosity of the Sun from its photosphere at an effective temperature of 6,276 K.[4]

A Jupiter-like planet has been detected in an eccentric orbit around this star via Doppler spectroscopy. The eccentricity of 0.27 indicates that the orbit carries the body from Script error: No such module "val". out to Script error: No such module "val". between periastron and apastron. The maximum surface temperature of the planet is ~400 K, varying by 100 K over the course of an orbit. There is a data trend in the results which may point to an additional companion further from its star, but this will require a longer observation period to validate.[9]

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See also

References

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Template:Sky Template:Stars of Piscis Austrinus