HD 40979

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HD 40979
Observation data
Equinox J2000.0
Constellation Auriga
Right ascension 06h 04m 29.9431s
Declination +44° 15' 37.599"
Apparent magnitude (V) +6.746
Distance 109 ly
(33 pc)
Spectral type F8V
Other designations
HIP 28767

HD 40979 is a yellow dwarf star about 109 light-years away in the constellation Auriga.

As of 2002 there is one extrasolar planet orbiting HD 40979.

Contents

[edit] Planet

[edit] HD 40979 b

HD 40979 b
Extrasolar planet Lists of extrasolar planets
Orbital elements
Semimajor axis (a) 0.855±0.049 AU
Eccentricity (e) 0.269±0.034
Orbital period (P) 263.84±0.71 d
Inclination (i)  ?°
Longitude of
periastron
(ω) 318±10°
Time of periastron (τ) 2,451,748.1
±8.6 JD
Physical characteristics
Mass (m) >3.83±0.36 MJ
Radius (r)  ? RJ
Density (ρ)  ? kg/m3
Temperature (T)  ? K
Discovery information
Discovery date 2002
Discoverer(s) Fischer et al.
Detection method Radial velocity
Discovery status Published

HD 40979 b is an extrasolar planet orbiting HD 40979. It is thought to be a large gas giant planet in the star's habitable zone with temperatures similar to Venus. It was discovered in 2002 by Debra Fischer.

[edit] References

[edit] External links



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