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Interstellar Objects and Exocomets

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arxiv 2303.17980 v1 pith:Q6UEACZL submitted 2023-03-31 astro-ph.EP astro-ph.GA

Interstellar Objects and Exocomets

classification astro-ph.EP astro-ph.GA
keywords exocometsinterstellaradvancescharacteristicsisoslookingobjectsstars
verification ladder T0 review T1 audit T2 compute T3 formal T4 reserved
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In this chapter we review our knowledge of our galaxy's cometary population outside our Oort Cloud - exocomets and Interstellar Objects (ISOs). We start with a brief overview of planetary system formation, viewed as a general process around stars. We then take a more detailed look at the creation and structure of exocometary belts, as revealed by the unprecedented combination of theoretical and observational advances in recent years. The existence and characteristics of individual exocomets orbiting other stars is summarized, before looking at the mechanisms by which they may be ejected into interstellar space. The discovery of the first two ISOs is then described, along with the surprising differences in their observed characteristics. We end by looking ahead to what advances may take place in the next decade.

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Cited by 1 Pith paper

Reviewed papers in the Pith corpus that reference this work. Sorted by Pith novelty score.

  1. NSF-DOE Vera C. Rubin Observatory Observations of Interstellar Comet 3I/ATLAS (C/2025 N1)

    astro-ph.EP 2025-07 accept novelty 4.0

    Rubin Observatory delivers the earliest large-telescope astrometry and grizy photometry of interstellar comet 3I/ATLAS, including colors and a dust-to-nucleus cross-section ratio lower limit.