Do planetary seasons play a role in attaining stable climates?

Kasper Wibeck Olsen, Jakob Bohr*

*Corresponding author for this work

    Research output: Contribution to journalJournal articleResearchpeer-review

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    A simple phenomenological account for planetary climate instabilities is presented. The description is based on the standard model where the balance of incoming stellar radiation and outward thermal radiation is described by the effective planet temperature. Often, it is found to have three different points, or temperatures, where the influx of radiation is balanced with the out-flux, even with conserved boundary conditions. Two of these points are relatively long- term stable, namely the point corresponding to a cold climate and the point corresponding to a hot climate. In a classical sense these points are equilibrium balance points. The hypothesis promoted in this paper is the possibility that the intermediate third point can become long-term stable by being driven dynamically. The initially unstable point is made relatively stable over a long period by the presence of seasonal climate variations.
    Original languageEnglish
    JournalMonthly Notices of the Royal Astronomical Society
    Issue number3
    Pages (from-to)3540-3543
    Publication statusPublished - 2018


    • Earth
    • Planetary systems


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