HD 108147 b
HD 108147 b is a gas giant exoplanet with a minimum mass about half that of Jupiter. It orbits the star in a very tight "torch orbit". The distance between the planet and the star is only a tenth of the distance between Earth and the Sun (0.1AU). A number of such worlds are known to exist, but the eccentricity of this planet is unusually high. Planets orbiting very close to their parent stars usually have round orbits because of the tidal forces between the bodies.
HD 108147 b
HD 108147 b is a gas giant exoplanet with a minimum mass about half that of Jupiter. It orbits the star in a very tight "torch orbit". The distance between the planet and the star is only a tenth of the distance between Earth and the Sun (0.1AU). A number of such worlds are known to exist, but the eccentricity of this planet is unusually high. Planets orbiting very close to their parent stars usually have round orbits because of the tidal forces between the bodies.
has abstract
HD 108147 b es un planeta extr ...... uerzas de marea entre cuerpos.
@es
HD 108147 b is a gas giant exo ...... dal forces between the bodies.
@en
HD 108147 b ist ein Exoplanet, ...... itermassen (ca. 83 Erdmassen).
@de
HD 108147 b è un pianeta extra ...... orze di marea tra i due corpi.
@it
HD 108147 b é um planeta extra ...... revolução em cerca de 11 dias.
@pt
HD 108147 b是一顆質量下限大約是木星一半質量的太陽 ...... 行星大多會因為兩者之間潮汐力的交互作用，使軌道相當接近圓形。
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Link from a Wikipage to an external page
Wikipage page ID
16.781.895
Wikipage revision ID
660.975.963
apastron
arg peri
colwidth
constell
discoverers
discovery date
2000-04-15
discovery method
discovery site
discovery status
dist ly
dist pc
eccentricity
minimum mass
minimum mass earth
periastron
period
period year
semi-amp
semimajor
t peri
2,4515916e+6
subject
hypernym
comment
HD 108147 b es un planeta extr ...... uerzas de marea entre cuerpos.
@es
HD 108147 b is a gas giant exo ...... dal forces between the bodies.
@en
HD 108147 b ist ein Exoplanet, ...... itermassen (ca. 83 Erdmassen).
@de
HD 108147 b è un pianeta extra ...... orze di marea tra i due corpi.
@it
HD 108147 b é um planeta extra ...... massivos conhecidos na época.
@pt
HD 108147 b是一顆質量下限大約是木星一半質量的太陽 ...... 行星大多會因為兩者之間潮汐力的交互作用，使軌道相當接近圓形。
@zh
label
HD 108147 b
@de
HD 108147 b
@en
HD 108147 b
@es
HD 108147 b
@it
HD 108147 b
@pt
HD 108147 b
@zh