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Photo-dynamical characterisation of the TOI-178 resonant chain

Photo-dynamical characterisation of the TOI-178 resonant chain

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3059644429

Photo-dynamical characterisation of the TOI-178 resonant chain

About this item

Full title

Photo-dynamical characterisation of the TOI-178 resonant chain

Publisher

Ithaca: Cornell University Library, arXiv.org

Journal title

arXiv.org, 2024-05

Language

English

Formats

Publication information

Publisher

Ithaca: Cornell University Library, arXiv.org

More information

Scope and Contents

Contents

The TOI-178 system consists of a nearby late K-dwarf transited by six planets in the super-Earth to mini-Neptune regime, with radii ranging from 1.2 to 2.9 earth radius and orbital periods between 1.9 and 20.7 days. All planets but the innermost one form a chain of Laplace resonances. The fine-tuning and fragility of such orbital configurations ens...

Alternative Titles

Full title

Photo-dynamical characterisation of the TOI-178 resonant chain

Identifiers

Primary Identifiers

Record Identifier

TN_cdi_proquest_journals_3059644429

Permalink

https://devfeature-collection.sl.nsw.gov.au/record/TN_cdi_proquest_journals_3059644429

Other Identifiers

E-ISSN

2331-8422

DOI

10.48550/arxiv.2405.13732

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