An exoplanet 50 light years away, with a radius twice that of Earth and eight times its mass, has a density of 5.52 g/cm³, suggesting a complex composition. The planet's density indicates it could have a significant iron core, a rocky mantle, and a higher water content compared to Earth. The challenge in determining its exact composition arises from having multiple variables—iron, rock, water, and hydrogen/helium—making it an underdetermined system. Comparisons to Uranus highlight that similar density can arise from different internal structures. Ultimately, the precise composition remains speculative due to the limitations of available data.