Earth Siblings Can Be Different: Chemical Clues on the Formation of Planetary Systems
An international team of researchers, with the participation of  IAC astronomers, has discovered that the chemical structure of  Earth-like planets can be very different from the bulk composition of  the Earth. This may have a dramatic effect on the existence and  formation of the biospheres and life on Earth-like planets.
The study of the photospheric stellar abundances of the planet-host  stars is the key to understanding how protoplanets form, as well as  which protoplanetary clouds evolve planets and which do not. These  studies, which have important implications for models of giant planet  formation and evolution, also help us to investigate the internal and  atmospheric structure and composition of extrasolar planets.
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Earth Siblings Can Be Different: Chemical Clues on the Formation of Planetary Systems

An international team of researchers, with the participation of IAC astronomers, has discovered that the chemical structure of Earth-like planets can be very different from the bulk composition of the Earth. This may have a dramatic effect on the existence and formation of the biospheres and life on Earth-like planets.

The study of the photospheric stellar abundances of the planet-host stars is the key to understanding how protoplanets form, as well as which protoplanetary clouds evolve planets and which do not. These studies, which have important implications for models of giant planet formation and evolution, also help us to investigate the internal and atmospheric structure and composition of .

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