HD 162020

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HD 162020
Observation data
Epoch J2000.0
Constellation
(pronunciation)
Scorpius
Right ascension 17h 50m 38.3575s
Declination −40º 19' 06.0562″
Apparent magnitude (V) +9.18
Absolute magnitude (V) +6.71
Distance 102.0 ly
(31.26 pc)
Spectral type K2V:
Other designations
CD−40 11894, HIP 87330

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

[edit] HD 162020 b

HD 162020 b
Extrasolar planet List of extrasolar planets
Orbital elements
Semimajor axis (a) 00751 AU
Eccentricity (e) 0.277 ± 0.02
Orbital period (P) 8.428198 ± 0.000056 d
Angular distance (θ) 2.40 mas
Longitude of
periastron
(ω) 28.40 ± 0.23°
Time of periastron (T0) 2451990.6768 ± 0.0050 JD
Semi-amplitude (K) 1813 ± 4 m/s
Physical characteristics
Mass (m) >15.0 MJ
Discovery information
Discovery date 2002
Discoverer(s) Udry et al.
Detection method Doppler Spectroscopy
Discovery site California, United States
Discovery status Published

HD 162020 b is a brown dwarf with mass 28.5 Wg (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 Earth-like planets around Gliese 581.

[edit] References

VIII. The very low-mass companions of HD 141937 , HD 162020 , HD 168443 and HD 202206 : Brown dwarfs or "superplanets"?]". Astronomy & Astrophysics 390: 267-279. 

[edit] External links