Close Cassini flybys of Saturn’s ring moons Pan, Daphnis, Atlas, Pandora, and Epimetheus

Author:

Buratti B. J.1ORCID,Thomas P. C.2,Roussos E.3ORCID,Howett C.4ORCID,Seiß M.5ORCID,Hendrix A. R.6,Helfenstein P.2ORCID,Brown R. H.7,Clark R. N.6,Denk T.8ORCID,Filacchione G.9ORCID,Hoffmann H.5ORCID,Jones G. H.10ORCID,Khawaja N.811,Kollmann P.11ORCID,Krupp N.3ORCID,Lunine J.2ORCID,Momary T. W.1ORCID,Paranicas C.12ORCID,Postberg F.811ORCID,Sachse M.5ORCID,Spahn F.5,Spencer J.4ORCID,Srama R.13ORCID,Albin T.13,Baines K. H.1,Ciarniello M.9ORCID,Economou T.14ORCID,Hsu H.-W.15ORCID,Kempf S.15ORCID,Krimigis S. M.12ORCID,Mitchell D.12ORCID,Moragas-Klostermeyer G.13ORCID,Nicholson P. D.2ORCID,Porco C. C.16,Rosenberg H.8ORCID,Simolka J.13ORCID,Soderblom L. A.17ORCID

Affiliation:

1. Jet Propulsion Laboratory, California Institute of Technology, Pasadena, CA 91109, USA.

2. Cornell Center for Astrophysics and Planetary Science, Cornell University, Ithaca, NY 14853, USA.

3. Max Planck Institute for Solar System Research, 37077 Göttingen, Germany.

4. Southwest Research Institute, Boulder, CO 80302, USA.

5. Department of Physics and Astronomy, University of Potsdam, 14476 Potsdam, Germany.

6. Planetary Sciences Institute, Tucson, AZ 85719, USA.

7. Lunar and Planetary Lab, University of Arizona, Tucson, AZ 85721, USA.

8. Institute of Geological Sciences, Freie Universität Berlin, 12249 Berlin, Germany.

9. Istituto Nazionale di Astrofisica, Rome, Italy.

10. University College London, London, UK.

11. Institute of Earth Sciences, University of Heidelberg, 69120 Heidelberg, Germany.

12. Applied Physics Laboratory, Johns Hopkins University, Laurel, MD 20723, USA.

13. University of Stuttgart, 70569 Stuttgart, Germany.

14. Enrico Fermi Institute, University of Chicago, Chicago, IL 60637, USA.

15. Physics Department, University of Colorado, Boulder, CO 80303, USA.

16. Space Sciences Institute, Boulder, CO 80301, USA, and Department of Astronomy, University of California, Berkeley, CA 94720, USA.

17. U.S. Geological Survey, Flagstaff, AZ 86001, USA.

Abstract

Cassini's last look at Saturn's rings During the final stages of the Cassini mission, the spacecraft flew between the planet and its rings, providing a new view on this spectacular system (see the Perspective by Ida). Setting the scene, Spilker reviews the numerous discoveries made using Cassini during the 13 years it spent orbiting Saturn. Iess et al. measured the gravitational pull on Cassini, separating the contributions from the planet and the rings. This allowed them to determine the interior structure of Saturn and the mass of its rings. Buratti et al. present observations of five small moons located in and around the rings. The moons each have distinctive shapes and compositions, owing to accretion of ring material. Tiscareno et al. observed the rings directly at close range, finding complex features sculpted by the gravitational interactions between moons and ring particles. Together, these results show that Saturn's rings are substantially younger than the planet itself and constrain models of their origin. Science , this issue p. 1046 , p. eaat2965 , p. eaat2349 , p. eaau1017 ; see also p. 1028

Funder

Science and Technology Facilities Council

Deutsches Zentrum für Luft- und Raumfahrt

German Research Foundation

NASA Cassini Project

German Space Agency

Cassini

Italian Space Agency

NASA Cassini

Publisher

American Association for the Advancement of Science (AAAS)

Subject

Multidisciplinary

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