HD 156668 b
Exoplanet | List of exoplanets | |
---|---|---|
Parent star | ||
Star | HD 156668 | |
Constellation | Hercules | |
Right ascension | (α) | 17h 17m 40s |
Declination | (δ) | +29° 13′ 38″ |
Apparent magnitude | (mV) | 8.42 |
Distance | 78.5 ± 2.0 ly (24.1 ± 0.6 pc) |
|
Spectral type | K2V | |
Physical characteristics | ||
Minimum mass | (m sin i) | 3.1 ± 0.4[1] M⊕ |
Orbital elements | ||
Semi-major axis | (a) | 0.04998 ± 0.00083[2] AU |
Eccentricity | (e) | 0.000[1] |
Orbital period | (P) | 4.6455 ± 0.0011[2] d |
Argument of periastron |
(ω) | 0[1]° |
Time of conjunction | (Tc) | 2454718.57 ± 0.11[2] JD |
Semi-amplitude | (K) | 1.89 ± 0.26 [2] m/s |
Discovery information | ||
Discovery date | 2010-01-06 | |
Discoverer(s) | Howard et al. | |
Discovery method | Doppler Spectroscopy | |
Discovery site | Keck Observatory | |
Discovery status | Submitted | |
Database references | ||
Extrasolar Planets Encyclopaedia |
data | |
SIMBAD | data | |
Exoplanet Archive | data | |
Open Exoplanet Catalogue | data |
HD 156668 b is an extrasolar planet orbiting the star HD 156668 78.5 light-years away in the constellation Hercules. It has a minimum mass of 3.1 Earth masses. At the time of discovery it was the second least massive planet discovered by the radial velocity method, subject to the mass/inclination degeneracy that affects radial velocity measurements.[3] The only radial velocity planet less massive than this planet is Gliese 581 e, which was discovered on April 21, 2009, and has a minimum mass of 1.94 Earth masses. In addition to this, it has the lowest semi-amplitude, or the speed of the stellar wobble caused by planet's gravity tugging on the star determined by radial velocity, at 2.2 m/s.[3] This planet was discovered on January 6, 2010; it is the 8th planet discovered in 2010 after the first five planets detected by Kepler on January 4 and two planets around HD 9446 on January 5.
References
<templatestyles src="Asbox/styles.css"></templatestyles>