HD 159868

HD 159868

Starbox short
name = HD 159868
constell = Scorpius
ra = RA|17|38|59.526
dec = DEC|-43|08|43.85
appmag_v = +7.24
absmag_v =
dist_ly = 171.93
dist_pc = 52.71
class = G5V
names = CD -43º 11901, GC 23898, GCRV 67207, GJ 4014, HD 159868, HIP 86375, SAO 228234
Simbad = HD+159868

HD 159868 is a yellow dwarf star approximately 172 light-years away in the constellation of Scorpius. The star is thought to be 3.05 times as luminous than the Sun, yet with the metallicity is identical to the Sun. As of 2007, an extrasolar planet has been confirmed to be orbiting the star.cite journal | url=http://www.journals.uchicago.edu/doi/abs/10.1086/513563 | author=O'Toole "et al." | title=New Planets around Three G Dwarfs | journal=The Astrophysical Journal | volume=660 | issue=2 | year=2007 | pages=1636 – 1641 | doi=10.1086/513563 ( [http://xxx.lanl.gov/abs/astro-ph/0702213 web Preprint] )]

Planetary system

In 2007, an extrasolar planet was announced by astronomer Simon J. O'Toole, to be orbiting the star. The planet (designated HD 159868 b) is likely to be a gas giant. The orbit is extremely eccentric at the average distance of 2 astronomical units (AU), ranging as close as 0.62 AU to as far as 3.38 AU. During its orbital period, the planet spends most of its time in the habitable zone of its star.

OrbitboxPlanet
exoplanet = b
mass = >1.7 ± 0.3
semimajor = 2 ± 0.3
period = 986 ± 9
eccentricity = 0.69 ± 0.02

See also

* HD 219828
* HD 28185
* List of stars with confirmed extrasolar planets

References

External links

*
*


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