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HD 175541 b image

HD 175541 b

World type: sub_neptune
Discovery method: Radial Velocity
Discovery year: 2007
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Meet Kavian, officially known as HD 175541 b, a charming exoplanet orbiting the star HD 175541. Discovered back in 2007 using the clever radial velocity technique with the HIRES Spectrometer at the W. M. Keck Observatory, Kavian represents a fascinating distant world explored from Earth’s vantage point. While it orbits its star at a comfortable distance, giving it unique qualities distinct from our own solar system, the specifics of its atmosphere and surface remain a playful cosmic mystery. Kavian’s discovery highlights the power of ground-based telescopes in unveiling the secrets of planets far beyond our reach, inviting us to dream about the diverse worlds that call our galaxy home.