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Detecting and Characterizing Exomoons and Exorings (Handbook of Exoplanets, 2nd Edition)

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arxiv 2401.13293 v1 pith:TRZL37BH submitted 2024-01-24 astro-ph.EP

classification astro-ph.EP
keywords exomoonsexoringsnumbersystemswillchallengescharacterizingcontributions
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The circumplanetary environments in our Solar System host a stunning array of moon and ring systems. Study of these environs has yielded valuable insights into planetary system formation and evolution, and there is every reason to believe that we will have much to learn from the moons and rings that are likely to exist in exoplanetary systems as well. This has motivated a small but growing number of researchers to investigate questions related to the formation, stability, long-term viability, composition, and observability of these exomoons and exorings. Still, due to a range of significant observational challenges, we remain at a relatively early stage of this work. As a result, we continue to face a number of difficult, unanswered questions, but this also means there are myriad opportunities for fundamental contributions to the field. In this review we will examine a variety of important issues for the astronomical community to consider, with an aim of providing a comprehensive understanding of ongoing efforts to identify and characterize exomoons and exorings, while also increasing interest and engagement. We begin with an overview of what we expect from systems hosting moons and/or rings in terms of their architectures, habitability, and observational signatures. We then highlight the contributions from a variety of works that have been aimed at detecting and characterizing them. We conclude by examining the outlook for finding these objects and discussing a number of ongoing challenges that we will want to overcome in the years ahead.

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Forward citations

Cited by 2 Pith papers

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score. OpenAlex reports about 3 citations worldwide. Full citation record

  1. On the formation of satellites in dense solid-particle disks

    astro-ph.EP 2025-07 conditional novelty 5.0 of 10

    In dense solid-particle disks, the mass of the largest formed satellite scales roughly linearly with disk mass, with a stochastic spread large enough that duplicated initial conditions produce very different moons.

  2. Highlights from Exoplanet Observations by the James Webb Space Telescope

    astro-ph.EP 2025-05 unverdicted novelty 3.0 of 10

    A review chapter of JWST exoplanet highlights with a compiled target database and reproducible figures.

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