# A New Line-By-Line General Circulation Model for Simulations of Diverse Planetary Atmospheres: Initial Validation and Application to the Exoplanet GJ 1132b

## TL;DR

This paper introduces a novel line-by-line 3D GCM for simulating diverse planetary atmospheres, validates it against existing models, and applies it to study the climate of the exoplanet GJ 1132b, revealing insights into atmospheric composition and circulation patterns.

## Contribution

The paper presents the first 3D GCM using a line-by-line radiative transfer approach, enhancing accuracy and flexibility for diverse planetary atmospheres.

## Key findings

- Minor CO2 can significantly alter circulation patterns.
- Phase shift of hotspot can reveal superrotating jet profiles.
- Oxygen-rich atmospheres' mass may be inferred from phase amplitude.

## Abstract

Exploring diverse planetary atmospheres requires modeling tools that are both accurate and flexible. Here, we develop a three-dimensional general circulation model (3D GCM) that for the first time uses a line-by-line approach to describe the radiative transfer. We validate our GCM by comparing with published results done by different 1D and 3D models. To demonstrate the versatility of the model, we apply the GCM to the hot Earth-sized exoplanet GJ 1132b and study its climate and circulation assuming an atmosphere dominated by abiotic oxygen (O$_2$). Our simulations show that a minor CO$_2$ composition can change the circulation pattern substantially, intensifying the equatorial superrotation in particular. Computation of the phase-resolved spectroscopy indicates that the vertical profile of the superrotating jet could be inferred in future spectro-photometric observations by the phase shift of the hotspot in the CO$_2$ principle absorption band centered at 667 cm$^{-1}$. We also show that atmospheric mass could potentially be constrained by the phase amplitude in the O$_2$ vibrational fundamental band for planets with O$_2$-rich atmospheres, although further experimental and/or theoretical O$_2$-O$_2$ collision-induced absorption data at high temperatures is needed to confirm this. More physical schemes such as moist dynamics will be implemented in the GCM in the future so that it can be used to tackle a wide variety of planetary climate problems.