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List of articles in "Celestial Body" category - Page 917

OGLE-2005-BLG-071Lb

OGLE-2005-BLG-071Lb is an planet discovered by the Optical Gravitational Lensing Experiment (OGLE) and others in 2005 using gravitational microlensing. According to the best fit model it has about 3.5 times […]


Cygnus OB2-12

Cygnus OB2 #12 is an extremely bright blue hypergiant with an absolute bolometric magnitude (all electromagnetic radiation) of โˆ’10.9 among the most luminous stars known in the galaxy. This makes […]


Gliese 86 b

Gliese 86 b sometimes referred to as Gliese 86 Ab[citation needed] (so as to distinguish the planet from companion star B) and or shortened to Gl 86 b is an […]


Gliese 317 b

Gliese 317 b is an extrasolar planet approximately 50 light-years away in the constellation of Pyxis. The planet was announced in July 2007 to be orbiting the red dwarf star […]


Gliese 674 b

Gliese 674 b is an extrasolar planet approximately 15 light years away in the constellation of Ara. This planet orbits tightly around Gliese 674. It is a sub-Neptune-or-Uranus-mass planet either […]


Gliese 849 b

Gliese 849 b is an extrasolar planet approximately 29 light years away in the constellation of Aquarius. It is the first long-period Jupiter-like planet discovered around a red dwarf announced […]


HD 219828 b

HD 219828 b is an extrasolar planet approximately 265 light years away in the constellation of Pegasus. This is a Neptune-mass planet at least 21 times more massive than Earth. […]


HD 159868 b

HD 159868 b is an extrasolar planet that orbits HD 159868. It is a jovian planet. The orbit is extremely eccentric at the average distance of 2 AU. The orbital […]


HD 23127 b

HD 23127 b is a jovian extrasolar planet orbiting the star HD 23127 at the distance of 2.29 AU taking 3.32 years to orbit. The orbit is very eccentric a […]


HD 47536 c

HD 47536 c is an extrasolar planet located approximately 396 light-years away in the constellation of Canis Major orbiting the star HD 47536. Like HD 47536 b mass and semimajor […]


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