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Habitable Zone Model for Low Metallicity Stars by InflatableOkapi is a document available to read on EtoBox.

This document presents a simple model to estimate the habitable zone around stars of various masses and lower metallicity than the Sun. It examines how metallicity affects the inner and outer habitable zone boundaries at the zero-age main sequence and terminal-age main sequence phases. The model finds that metallicity has little impact on the habitable zone range early in a star

Author
InflatableOkapi
Language
EN