Terrestrial planets across space and time
E. Zackrisson, P. Calissendorff, J. Gonzalez, A. Benson, A. Johansen,, M. Janson

TL;DR
This paper models the distribution and age of terrestrial planets across cosmic history, estimating their total numbers and examining factors affecting their habitability and detection prospects.
Contribution
It introduces a coupled semi-analytic model linking galaxy formation to planet occurrence, providing a comprehensive cosmic inventory of terrestrial planets and their ages.
Findings
Mean age of terrestrial planets: 7-8 Gyr in the local Universe.
Estimated total terrestrial planets: ~10^19 around FGK stars, ~5x10^20 around M stars.
Less than 10% of terrestrial planets are affected by hot Jupiters.
Abstract
The study of cosmology, galaxy formation and exoplanets has now advanced to a stage where a cosmic inventory of terrestrial planets may be attempted. By coupling semi-analytic models of galaxy formation to a recipe that relates the occurrence of planets to the mass and metallicity of their host stars, we trace the population of terrestrial planets around both solar-mass (FGK type) and lower-mass (M dwarf) stars throughout all of cosmic history. We find that the mean age of terrestrial planets in the local Universe is Gyr for FGK hosts and Gyr for M dwarfs. We estimate that hot Jupiters have depleted the population of terrestrial planets around FGK stars by no more than , and that only of the terrestrial planets at the current epoch are orbiting stars in a metallicity range for which such planets have yet to be confirmed. The typical…
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