the Creative Commons Attribution 4.0 License.
the Creative Commons Attribution 4.0 License.
ROCKE-3D 2.0: An updated general circulation model for simulating the climates of rocky planets
Abstract. We present the second generation of ROCKE-3D (Resolving Orbital and Climate Keys of Earth and Extraterrestrial Environments with Dynamics), a generalized 3-dimensional General Circulation Model (GCM) for use in Solar System and exoplanetary simulations of rocky planet climates. ROCKE-3D version 2.0 is a descendant of ModelE2.1, the flagship Earth System Model of the NASA Goddard Institute for Space Studies (GISS) used in the most recent Intergovernmental Panel for Climate Change (IPCC) assessments. ROCKE-3D is a continuous effort to expand the capabilities of GISS ModelE to handle a broader range of planetary conditions, including different atmospheric planet sizes, gravities, pressures, rotation rates, more diverse chemistry schemes and atmospheric compositions, diverse ocean and land distributions and topographies, and potential basic biosphere functions. In this release we present updated physics, and many more supported configurations which can serve as starting points to simulate the atmospheres of rocky terrestrial planets of interest. Two different radiation schemes are supported, the GISS radiation, valid only for atmospheres similar to that of modern Earth, and SOCRATES , which is more generalized but more computationally expensive. While ROCKE-3D can simulate a very wide range of planetary and atmospheric configurations, we describe here a small subset of them, with the goal of demonstrating the structural capabilities, rather than the scientific breadth, of the model. Three different atmospheric composition options are described (preindustrial Earth, the atmosphere used in ROCKE-3D 1.0, and an anoxic atmosphere with no aerosols), three ocean configurations (prescribed, Q-flux, and dynamic), and two resolutions: the medium resolution (4x5 degrees in latitude and longitude, previously used in ROCKE-3D 1.0), and the fine resolution, which has double the resolution in the atmosphere and 4 times the horizontal and 3 times the vertical resolution in the ocean. Finally, for the land surface hydrology, we have introduced generalized physics for arbitrary topography in the pooling and evaporation of water and river transport of water between grid cells, and for the vertical stratification of temperature in dynamic lakes. We quantify how the different component choices affect model results, and discuss strengths and limitations of using each component, together with how one can select which component to use. ROCKE-3D is publicly available and tutorial sessions are available for the community, greatly facilitating its use by any interested group.
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Status: open (until 12 May 2025)
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CEC1: 'Comment on egusphere-2025-925', Juan Antonio Añel, 21 Mar 2025
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Dear authors,
Unfortunately, after checking your manuscript, it has come to our attention that it does not comply with our "Code and Data Policy".
https://www.geoscientific-model-development.net/policies/code_and_data_policy.htmlYou have archived the ROCKE-3D code in a site that does not comply with our code policy. Therefore, please publish your code in one of the appropriate repositories according to our policy.
In this way, you must reply to this comment with the link to the new repository used in your manuscript, and its permanent identifier (e.g. DOI). The reply and the repository should be available as soon as possible, and before the Discussions stage is closed, to be sure that anyone has access to it for review purposes.Please, note that if you do not fix this problem, we will have to reject your manuscript for publication in our journal.
Juan A. Añel
Geosci. Model Dev. Executive EditorCitation: https://doi.org/10.5194/egusphere-2025-925-CEC1 -
AC1: 'Reply on CEC1', Kostas Tsigaridis, 22 Mar 2025
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Dear executive editor,
Thank you for your comment. The model code is already stored in the zenodo public archive together with our simulation output, which contains a DOI. This is mentioned in lines 95-96 of the submitted manuscript:
“The model code, all output, and the model configurations used here, are available on a zenodo archive (Tsigaridis et al., 2025)”
This is mentioned in the zenodo metadata too:
“modelE2_planet_2.0.tar.gz: The model code. This is identical to the code provided in the official model snapshots website (https://simplex.giss.nasa.gov/snapshots/) under "version 2.0 of ROCKE-3D model"”
We do acknowledge though that we failed to report this in the code availability section of the manuscript, which only points to our long-term institutional repository that has no DOI associated with it. In the revised version we will include a statement about the zenodo availability there as well.
Kostas Tsigaridis, on behalf of all co-authors.
Citation: https://doi.org/10.5194/egusphere-2025-925-AC1 -
CEC2: 'Reply on AC1', Juan Antonio Añel, 23 Mar 2025
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Dear authors,
Thanks for pointing it out. Please, as you say, in any reviewed version of the manuscript include the information on the repository on the section that corresponds to it. It would be good that you remove the link to the NASA site. The goal of the Code Availability section is not to promote the last version of a model or an institution, but to provide the exact assets used to perform a research, and comply with the replicability that the scientific method requests. Including a link to a site that does not comply with such goal and that is not assured to be available in the future, only introduces unnecessary noise.
Juan A. Añel
Geosci. Model Dev. Executive Editor
Citation: https://doi.org/10.5194/egusphere-2025-925-CEC2
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CEC2: 'Reply on AC1', Juan Antonio Añel, 23 Mar 2025
reply
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AC1: 'Reply on CEC1', Kostas Tsigaridis, 22 Mar 2025
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