HD 162020

HD 162020

Starbox short
name = HD 162020
epoch = J2000.0
constell = Scorpius
ra = 17h 50m 38.3575s
dec = −40º 19' 06.0562″
spectral = K2V:
appmag_v = +9.18
absmag_v = +6.71
dist_ly = 102.0
dist_pc = 31.26
names = CD−40 11894, HIP 87330

HD 162020 is an orange dwarf star in Scorpius constellation with a brown dwarf companion.

HD 162020 b

Planetbox begin
name = HD 162020 b
Planetbox orbit
semimajor = 00751
eccentricity = 0.277 ± 0.02
period = 8.428198 ± 0.000056
ang_dist = 2.40
long_peri = 28.40 ± 0.23
t_peri = 2451990.6768 ± 0.0050
semi-amp = 1813 ± 4
Planetbox character
mass = >15.0
Planetbox discovery
discovery_date = 2002
discoverers = Udry et al.
discovery_method = Doppler Spectroscopy
discovery_site = California, United States
discovery_status=Published
HD 162020 b is a brown dwarf with mass 15.0 MJ. The mass is minimum since inclination is not known. This planetar orbits very close to the star at a distance of 0.075 AU. Despite of this, it has an eccentric orbit of 27.7%. The distance from the star ranges from 0.054 to 0.096 AU. It has an extremely high semi-amplitude of 1813 m/s.

In 2002, Stephen Udry discovered HD 162020 b taking place in California. Udry was the same person who discovered two super-Earth planets orbiting around Gliese 581.

References

* cite journal |url=http://www.aanda.org/index.php?option=article&access=standard&Itemid=129&url=/articles/aa/abs/2002/28/aa2416/aa2416.html |author=Udry et al. |title=The CORALIE survey for southern extra-solar planetsVIII. The very low-mass companions of HD 141937 , HD 162020 , HD 168443 and HD 202206 : Brown dwarfs or "superplanets"?
journal=Astronomy & Astrophysics |eprint= |class=astro-ph |year=2002 |volume=390 |issue= |pages=267–279 |accessdate=December 21 |accessyear=2007

External links

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