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ABSTRACT We present here evidence that two previously unidentified, yet conspicuous gaps in Saturn's rings lie at distances corresponding to 2/3 and 4/3 of the planet's rotation
period. Gaps such as these can be produced in a ring of large bodies or small uncharged particles only by a non-axisymmetric gravitational field (both of the above can be associated with the
_l_ = _m_ = 3 harmonic), a fact that is relevant to models of planetary interiors. Access through your institution Buy or subscribe This is a preview of subscription content, access via
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* Learn about institutional subscriptions * Read our FAQs * Contact customer support SIMILAR CONTENT BEING VIEWED BY OTHERS A DENSE RING OF THE TRANS-NEPTUNIAN OBJECT QUAOAR OUTSIDE ITS
ROCHE LIMIT Article 08 February 2023 PLANETESIMAL RINGS AS THE CAUSE OF THE SOLAR SYSTEM’S PLANETARY ARCHITECTURE Article 30 December 2021 GRAVITATIONAL INSTABILITY IN A PLANET-FORMING DISK
Article 04 September 2024 REFERENCES * Collins, S. A. _et al._ _Nature_ 288, 439–442 (1980). Article ADS Google Scholar * Goldreich, P. & Tremaine, S. _Icarus_ 34, 240 (1978). Article
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Cambridge, Massachusetts, 02138, USA F. A. Franklin, G. Colombo & A. F. Cook Authors * F. A. Franklin View author publications You can also search for this author inPubMed Google Scholar
* G. Colombo View author publications You can also search for this author inPubMed Google Scholar * A. F. Cook View author publications You can also search for this author inPubMed Google
Scholar RIGHTS AND PERMISSIONS Reprints and permissions ABOUT THIS ARTICLE CITE THIS ARTICLE Franklin, F., Colombo, G. & Cook, A. A possible link between the rotation of Saturn and its
ring structure. _Nature_ 295, 128–130 (1982). https://doi.org/10.1038/295128a0 Download citation * Received: 19 August 1981 * Accepted: 13 November 1981 * Issue Date: 14 January 1982 * DOI:
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