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Encounter with Saturn: Voyager 1 Imaging Science Results
Abstract
As Voyager 1 flew through the Saturn system it returned photographs revealing many new and surprising characteristics of this complicated community of bodies. Saturn's atmosphere has numerous, low-contrast, discrete cloud features and a pattern of circulation significantly different from that of Jupiter. Titan is shrouded in a haze layer that varies in thickness and appearance. Among the icy satellites there is considerable variety in density, albedo, and surface morphology and substantial evidence for endogenic surface modification. Trends in density and crater characteristics are quite unlike those of the Galilean satellites. Small inner satellites, three of which were discovered in Voyager images, interact gravitationally with one another and with the ring particles in ways not observed elsewhere in the solar system. Saturn's broad A, B, and C rings contain hundreds of "ringlets," and in the densest portion of the B ring there are numerous nonaxisymmetric features. The narrow F ring has three components which, in at least one instance, are kinked and crisscrossed. Two rings are observed beyond the F ring, and material is seen between the C ring and the planet.
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Metadata
- Authors
- Smith, B. A., Soderblom, L., Beebe, R., Boyce, J., Briggs, G., Bunker, A., Collins, S. A., Hansen, C. J., Johnson, T. V., Mitchell, J. L., Terrile, R. J., Carr, M., Cook, A. F., Cuzzi, J., Pollack, J. B., Danielson, G. E., Ingersoll, A., Davies, M. E., Hunt, G. E., Masursky, H., Shoemaker, E., Morrison, D., Owen, T., Sagan, C., Veverka, J., Strom, R., & Suomi, V. E.
- Affiliations
- University of Arizona (US)
- United States Geological Survey (US)
- New Mexico State University (US)
- National Aeronautics and Space Administration (US)
- California Institute of Technology (US)
- University of Hawaii System (US)
- ORCID
- Venue
- Science
- Published
- 1981-04-10
- Volume
- 212
- Issue
- 4491
- Pages
- 163-191
- ISSN
- 0036-8075 (ISSN-L)
- 1095-9203
- OpenAlex
- W1998543912
- Cited by
- 795
- References
- 67
- Citations by year
- 2026: 8 · 2025: 12 · 2024: 22 · 2023: 20 · 2022: 9 · 2021: 13 · 2020: 13 · 2019: 17 · 2018: 16 · 2017: 15 · 2016: 14 · 2015: 15 · 2014: 10 · 2013: 10 · 2012: 13
- FWCI
- 111.60
- Type
- journal article
- Language
- en
- Open access
- closed
- Locations
- Science (publishedVersion)
- PubMed (publishedVersion)
- CaltechAUTHORS (California Institute of Technology) (submittedVersion)
- Topics
- Physical Sciences › Earth and Planetary Sciences › Space and Planetary Science › Astro and Planetary Science
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › Stellar, planetary, and galactic studies
- Physical Sciences › Physics and Astronomy › Astronomy and Astrophysics › History and Developments in Astronomy
- Keywords
- Saturn, Voyager 1, Saturn atmosphere, Titan haze, icy satellites, ringlets, Saturn rings, f-rings, satellite density, crater formation, planetary atmospheres
About these checks
Registry, retraction, Cites and statistics results are computed, not judged, with one exception: a printed reference that no index lists is read once by a model before it counts as a citation error. Claims are extracted by a model and kept only when their quote appears verbatim in the text; each cited source is then checked, with a model’s help, for whether it says what the claim relies on. Those verdicts can be wrong — read the claim’s quote and the cited source before relying on one.
Statistics and arithmetic are recomputed, not judged.
Confidence bands are shown only for fields calibrated on our annotated test set. None is calibrated yet, so no band is shown.
What counts as a claim ›How we measure confidence ›How we check this ›
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