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Constraints from Planets in Binaries

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Formation, Evolution, and Dynamics of Young Solar Systems

Part of the book series: Astrophysics and Space Science Library ((ASSL,volume 445))

Abstract

In this chapter I will discuss how planets place powerful constraints on the formation and early evolution of binary star systems. In addition, these systems demonstrate extreme modes of planet formation that can inform models of our own Solar System. I begin with a very brief overview of the theoretical mechanisms for forming binaries and their planets. I will present as case studies two triple-star systems comprising at least one planet orbiting one of the stars. Combining the information from these studies reveals that (1) many binaries with periods of 10–100 s of days form in their current orbital configurations as part of the star formation process (2) the frequency of tertiary companions in close binary systems may be indicative of three body instabilities other than the Kozai-Lidov mechanism (3) planet formation can proceed in highly perturbed, truncated disks, (4) a reservoir of material beyond the ice line may not be required to instigate planet formation.

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Acknowledgements

KMK is supported by the National Science Foundation under Grant No. AST-1410174.

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  1. Department of Astronomy, University of Arizona, 933 N Cherry Avenue, Tucson, AZ, 85721, USA

    Kaitlin M. Kratter

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  1. The Niels Bohr Institute, Niels Bohr International Academy, Copenhagen, Denmark

    Martin Pessah

  2. The Niels Bohr Institute, Niels Bohr International Academy, Copenhagen, Denmark

    Oliver Gressel

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Kratter, K.M. (2017). Constraints from Planets in Binaries. In: Pessah, M., Gressel, O. (eds) Formation, Evolution, and Dynamics of Young Solar Systems. Astrophysics and Space Science Library, vol 445. Springer, Cham. https://doi.org/10.1007/978-3-319-60609-5_11

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