NFT token detail for exoplanet HD 62509 b. Only at exoplanetary.systems.

HD 62509 b is a sub_neptune exoplanet discovered in 2006 using the Radial Velocity method.

HD 62509 b image

HD 62509 b

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Discovery Details

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2006
Facility: Multiple Observatories
Instrument: Multiple Instruments
Telescope: Multiple Telescopes
HD 62509 b is a fascinating giant exoplanet orbiting the bright star HD 62509, also known as Pollux, a comfortable stone's throw away in the constellation Gemini. Discovered in 2006 using the trusty radial velocity technique across multiple ground-based observatories, this celestial heavyweight shows us how stars can have their own planetary dance partners. Though we don’t have a catchy nickname for this planet yet, its presence around Pollux—a star easily visible to the naked eye—makes it a stellar neighbor worth knowing about. Imagine a giant world circling a well-loved star, quietly spinning through space while we, here on Earth, eagerly watch and learn from our many instruments aiming at the Gemini skies. It’s a brilliant example of the many diverse worlds out there waiting to be explored!