Eccentric orbits may enhance the habitability of Earth-like exoplanets

The detection and characterization of Earth-like planets around Sun-like stars is a crucial goal of exoplanetary research, given their promise for hosting potentially habitable conditions. Key orbital parameters, such as eccentricity, can influence a planet's climate response and, as a consequence, affect its potential habitability. Utilizing the Earth-system model - the Whole Atmosphere Community Climate Model (WACCM6), we simulated Earth-like exoplanets with two different orbital parameters: one circular (e = 0) and another highly eccentric (e = 0.4), both with zero obliquity but fixing the annual mean insolation. The highly eccentric case exhibits a 1.9 K warmer surface temperature due to lower surface and cloud albedo and a weaker longwave cloud forcing. Exploring the annual global mean climate difference, we analyzed latitudinal and seasonal variations in hydrological cycle variables, such as sea ice, land snow, and clouds. Land habitability metrics based on temperature and precipi..., The netCDF (.nc files) data were produced from simulations using the WACCM6 (CESM2.1.3) model.
See https://www2.acom.ucar.edu/gcm/waccm and https://doi.org/10.1029/2019JD030943 for more information.
These simulations were performed on the ARC4 HPC at the University of Leeds.
The output variables from the simulations are monthly mean files (h0.files) grouped in two folders for the circular (e=0) and eccentric cases (e=0.4).
To produce the figures in the manuscript, Python programming language was used along with the xarray packages., , # Eccentric orbits may enhance the habitability of Earth-like exoplanets

[https://doi.org/10.5061/dryad.2fqz612x7](https://doi.org/10.5061/dryad.2fqz612x7)

The datasets include multiple variables which are generated using WACCM6 in pre-industrial configuration with a 2-degree horizontal resolution and a simplified middle atmosphere chemistry (See [https://www2.acom.ucar.edu/gcm/waccm](https://www2.acom.ucar.edu/gcm/waccm) and [https://doi.org/10.1029/2019JD030943](https://doi.org/10.1029/2019JD030943) for more information.)

## Description of the data and file structure

The datasets are divided into two folders, one for the high-eccentric orbit (`e=0.4`) and another for the circular orbit case (`e=0`). Each folder has the same list of variable outputs in netCDF format (.nc files). The netCDF (.nc files) data were produced from simulations using the WACCM6 (CESM2.1.3) model.

The file names in each folder indicate the variable names, followed by the simulation case's name abbreviation...