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INAF-led study identifies two distinct families of multi-planet systems

An international research team led by the National Institute for Astrophysics (INAF) has identified two distinct families of multi-planet systems in the Milky Way. The study, published in Nature Astronomy, reveals a direct link between a host star's properties and the architecture and dynamic evolution of its planetary systems.

By analyzing 300 well-characterized systems, researchers found that the first family consists of large, massive systems orbiting massive, metal-rich stars. These systems often have total masses between two and ten times that of the Solar System.

The second family comprises compact, lower-mass systems orbiting stars with mass and metallicity equal to or lower than the Sun. These systems feature planets of similar size and mass, a configuration described as 'peas-in-a-pod,' orbiting at much closer distances than Mercury orbits the Sun.

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Milky Way · National Institute for Astrophysics · Nature Astronomy

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