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Publication Abstracts

Tsigaridis et al. 2025, submitted

Tsigaridis, K., A.S. Ackerman, I. Aleinov, M.A. Chandler, T.L. Clune, C.M. Colose, A.D. Del Genio, M. Kelley, N.Y. Kiang, A. Leboissetier, J.P. Perlwitz, R.A. Ruedy, G.L. Russell, L.E. Sohl, M.J. Way, and E.T. Wolf, 2025: ROCKE-3D 2.0: An updated general circulation model for simulating the climates of rocky planets. Geosci. Model Dev., submitted.

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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BibTeX Citation

@unpublished{ts02400q,
  author={Tsigaridis, K. and Ackerman, A. S. and Aleinov, I. and Chandler, M. A. and Clune, T. L. and Colose, C. M. and Del Genio, A. D. and Kelley, M. and Kiang, N. Y. and Leboissetier, A. and Perlwitz, J. P. and Ruedy, R. A. and Russell, G. L. and Sohl, L. E. and Way, M. J. and Wolf, E. T.},
  title={ROCKE-3D 2.0: An updated general circulation model for simulating the climates of rocky planets},
  year={2025},
  journal={Geoscientific Model Development},
  note={Manuscript submitted for publication}
}

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RIS Citation

TY  - UNPB
ID  - ts02400q
AU  - Tsigaridis, K.
AU  - Ackerman, A. S.
AU  - Aleinov, I.
AU  - Chandler, M. A.
AU  - Clune, T. L.
AU  - Colose, C. M.
AU  - Del Genio, A. D.
AU  - Kelley, M.
AU  - Kiang, N. Y.
AU  - Leboissetier, A.
AU  - Perlwitz, J. P.
AU  - Ruedy, R. A.
AU  - Russell, G. L.
AU  - Sohl, L. E.
AU  - Way, M. J.
AU  - Wolf, E. T.
PY  - 2025
TI  - ROCKE-3D 2.0: An updated general circulation model for simulating the climates of rocky planets
JA  - Geosci. Model Dev.
JO  - Geoscientific Model Development
ER  -

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