{ "cells": [ { "cell_type": "markdown", "id": "178c0a2a", "metadata": {}, "source": [ "# Thermal Emission Retrievals of Bare Rocky Exoplanets \n", "\n", "Tidally locked, hot, bare-rocky exoplanets provide a unique avenue to explore surface geology by probing mid-infrared absorption features characteristc of specific rocks.\n", "\n", "In this tutorial, we explore how to perform retrieval analysis when assuming a bare rocky exoplanet with no atmosphere (though, we note that all the surface + atmosphere + clouds models featured in 'Rocky Planets with Reflecting and Emitting Surfaces' can be used in a retrieval, here we only explore planetary bodies without atmospheres in since, as we will see below, the retrieval run very fast compared to models with atmospheres and clouds). \n", "\n", "This tutorial assumes a basic understanding of the 'Atmospheric Retrievals with POSEIDON' tutorial. " ] }, { "cell_type": "markdown", "id": "89224c6f", "metadata": {}, "source": [ "