description HD 114762 Overview
HD 114762 is a solar-type star located approximately 132 light-years from Earth in the constellation Coma Berenices. It gained significant astronomical attention in 1989 when researchers announced the discovery of a substellar companion orbiting it, making it one of the first stars outside our solar system found to have a massive orbiting body. The companion is thought to be either a large exoplanet or a brown dwarf. HD 114762 remains an important point of study for astrophysicists researching early planetary detection methods.
help HD 114762 FAQ
Where is the star HD 114762 located in the night sky?
HD 114762 is a solar-type star located approximately 132 light-years away from Earth. It can be found in the northern sky within the borders of the constellation Coma Berenices.
Why is HD 114762 important in the history of astronomy?
HD 114762 gained significant attention in 1989 when researchers announced the discovery of a substellar companion orbiting it. This made it one of the very first stars ever found to host a planet-like object, predating many major exoplanet discoveries.
Is HD 114762 similar to our own Sun?
Yes, HD 114762 is classified as a solar-type star, meaning it shares many fundamental physical characteristics with our Sun. It serves as an important point of comparison for scientists studying stellar evolution and solar analogs.
What exactly is orbiting around HD 114762?
The object orbiting HD 114762 is a substellar companion, which astronomers believe is likely a brown dwarf or a massive gas giant planet. Its exact classification has been a topic of scientific debate since its late-1980s discovery.
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