Studies of 15 M-type stars have revealed new insights into the potential presence of exoplanets. A new study led by astronomers at Heidelberg University reveals that Earth-like planets may be much more common than we thought, especially around small, low-mass stars. Using data from the CARMENES project, an international team discovered four new exoplanets and […]



Summary

A Heidelberg University study of 15 M-type stars, leveraging data from the CARMENES project, suggests Earth-like exoplanets may be more prevalent around small, low-mass stars than previously believed. The research resulted in the discovery of four new exoplanets. This finding challenges previous assumptions about planetary formation and habitability, suggesting that M-dwarf stars could be promising locations in the search for potentially habitable worlds. Further research is needed to confirm their characteristics.

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