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HD 1690 b image

HD 1690 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2010
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HD 1690 b is a fascinating giant exoplanet orbiting the star HD 1690, discovered back in 2010 by the clever use of the radial velocity method with the trusty HARPS Spectrograph at La Silla Observatory. This distant world, found using ground-based observations, offers an intriguing glimpse into planetary systems far beyond our own. Though it doesn’t have a fancy proper name yet, HD 1690 b stands as a testament to the power of precision instruments and patient astronomers. While we might not know all its details, imagining this massive planet circling its star is a delightful reminder of the vast, diverse cosmos waiting to be explored. A cosmic neighbor in the night sky, it sparks curiosity and wonder for all space enthusiasts!