description HD 28185 Overview
HD 28185 is a yellow dwarf star located approximately 138 light-years away in the constellation Eridanus, classified as a G-type solar analog. It is known for hosting an exoplanet, HD 28185 b, which was discovered in 2001 by the CORALIE spectrograph team using the radial velocity method. The exoplanet is a gas giant that orbits within the star's habitable zone, prompting ongoing scientific discussion regarding the potential habitability of any exomoons it might possess. The star itself contains a similar metallicity to the Sun.
help HD 28185 FAQ
Does the star HD 28185 have any exoplanets?
Yes, HD 28185 is known to host an exoplanet called HD 28185 b, which was discovered in 2001. The planet was detected using the radial velocity method by the CORALIE spectrograph team.
What type of star is HD 28185?
HD 28185 is classified as a G-type yellow dwarf star, making it a close solar analog to our own Sun. This solar-like nature makes it a prime target for astronomers studying planetary system formation.
How far away is the HD 28185 star system?
The star is located approximately 138 light-years away from Earth. It resides within the boundaries of the southern constellation Eridanus.
How was the planet around HD 28185 discovered?
The exoplanet HD 28185 b was discovered in 2001 using the radial velocity method. Astronomers utilized the CORALIE spectrograph to measure the subtle gravitational wobble of the star caused by the orbiting planet.
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