TOI 849 b is considered a sub-Neptune or a Super-Earth. However, it stands out due to its composition and location. With a radius approximately 3.45 times that of Earth and a mass around 40 times greater, TOI 849 b has a density similar to Earth's, suggesting a rocky composition. This is unusual for planets of its size, which are typically gas giants. Additionally, its close proximity to its host star places it in the hot Neptune desert, a region where such planets are rarely found.
