HD 154345 b

HD 154345 b
Extrasolar planet List of extrasolar planets

HD 154345 b and a hypothetical rocky moon.
(Artist's impression)
Parent star
Star HD 154345
Constellation Hercules
Right ascension (α) 17h 02m 36.40s
Declination (δ) +47° 04′ 54.77″
Apparent magnitude (mV) 6.74
Distance 58.91 ± 0.59 ly
(18.06 ± 0.18 pc)
Spectral type G8V
Mass (m) 0.88 M
Orbital elements
Semimajor axis (a) 4.18 AU
(625 Gm)
    89.9 mas
Periastron (q) 4.03 AU
(603 Gm)
Apastron (Q) 4.33 AU
(647 Gm)
Eccentricity (e) 0.036 ± 0.046
Orbital period (P) 3322 ± 93 d
(9.095 y)
Orbital speed (υ) 13.7 km/s
Argument of
periastron
(ω) 113°
Time of periastron (T0) 2,453,230 ± 330 JD
Semi-amplitude (K) 14.28 ± 0.75 m/s
Physical characteristics
Minimum mass (m sin i) 0.963 MJ
Discovery information
Discovery date March 12, 2006
(confirmed: May 27, 2007)
Discoverer(s) Wright et al.
Detection method radial velocity
Discovery site United States
Discovery status published
Other designations
Gliese 651 b, HIP 83389 b, SAO 46452 b
Database references
Extrasolar Planets
Encyclopaedia
data
SIMBAD data

HD 154345 b, is a Jupiter-sized extrasolar planet orbiting the star HD 154345.

Contents

Discovery

Wright et al. discovered the planet in March 2006 using the radial velocity method to detect the small wobbling movement of the star caused by the gravity of the planet. The discovery was confirmed in May 2007.[1]

Characteristics

The planet is a gas giant with a mass at least slightly less than that of Jupiter and is likely to be a near twin of Jupiter, estimated to be around the same size, or slightly larger. It may also harbor a system of moons and rings. It orbits its parent star at the distance of 4.18 AU. Its orbital period is about 9.095 Earth years and its orbit is circular.[2]

See also

References

Coordinates: 17h 02m 36.40s, +47° 04′ 54.77″