HD 205739

HD 205739 is a yellow-white dwarf (spectral type F7 V). It is about 108 parsecs away from the Sun.[1]

HD 205739
Observation data
Epoch J2000.0      Equinox J2000.0
Constellation Piscis Austrinus
Right ascension  21h 38m 08.404s[1]
Declination −31° 44 14.96 [1]
Apparent magnitude (V) 8.56
Characteristics
Spectral type F7 V
B−V color index 0.546
Astrometry
Radial velocity (Rv)9.1 km/s
Proper motion (μ) RA: 20.94 ± 0.90[1] mas/yr
Dec.: -83.69 ± 0.53[1] mas/yr
Parallax (π)9.28 ± 0.84[1] mas
Distance350 ± 30 ly
(108 ± 10 pc)
Absolute magnitude (MV)3.78
Details
Mass1.22 M
Radius1.33 R
Luminosity2.3 L
Temperature6176 ± 45 K
Metallicity+0.19 ± 0.04
Age2.84 Gyr years
Other designations
CD−32° 16667, HIP 106824, SAO 213152, PPM 301636
Database references
SIMBADdata
Extrasolar Planets
Encyclopaedia
data

The star HD 205739 is named Sāmaya. The name was selected in the NameExoWorlds campaign by Sri Lanka, during the 100th anniversary of the IAU. Sāmaya means peace in the Sinhalese language.[2][3]

A Jupiter-like planet has recently been detected in a Mercury-like eccentric orbit around this star.

There is a trend in the results which may point to an additional companion further from its star.[4]

The HD 205739 planetary system[4]
Companion
(in order from star)
Mass Semimajor axis
(AU)
Orbital period
(days)
Eccentricity Inclination Radius
b >1.37 MJ 0.896 279.8 ± 0.1 0.27 ± 0.07

See also

References

  1. van Leeuwen, F. (2007). "Validation of the new Hipparcos reduction". Astronomy and Astrophysics. 474 (2): 653–664. arXiv:0708.1752. Bibcode:2007A&A...474..653V. doi:10.1051/0004-6361:20078357. Vizier catalog entry
  2. "Approved names". NameExoworlds. Retrieved 2020-01-02.
  3. "International Astronomical Union | IAU". www.iau.org. Retrieved 2020-01-02.
  4. López-Morales, Mercedes; et al. (2008). "Two Jupiter-Mass Planets Orbiting HD 154672 and HD 205739". The Astronomical Journal. 136 (5): 1901–1905. arXiv:0809.1037. Bibcode:2008AJ....136.1901L. doi:10.1088/0004-6256/136/5/1901.


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