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Science 29 January 1982:
Vol. 215. no. 4532, pp. 537 - 543
DOI: 10.1126/science.215.4532.537

Articles

Photopolarimetry from Voyager 2; Preliminary Results on Saturn, Titan, and the Rings

ARTHUR L. LANE 1, CHARLES W. HORD 2, ROBERT A. WEST 2, LARRY W. ESPOSITO 2, DAVID L. COFFEEN 3, MAKIKO SATO 3, KAREN E. SIMMONS 4, RICHARD B. POMPHREY 5, and RICHARD B. MORRIS 5

1 Jet Propulsion Laboratory, California Institute of Technology, Pasadena 91109
2 Laboratory for Atmospheric and Space Physics, University of Colorado, Boulder 80309
3 Goddard Institute for Space Studies, New York 10025
4 Laboratory for Atmospheric and Space Physics, University of Colorado
5 Jet Propulsion Laboratory, California Institute of Technology

The Voyager 2 photopolarimeter was reprogrammed prior to the August 1981 Saturn encounter to perform orthogonal-polarization, two-color measurements on Saturn, Titan, and the rings. Saturn's atmosphere has ultraviolet limb brightening in the mid-latitudes and pronounced polar darkening north of 65°N. Titan's opaque atmosphere shows strong positive polarization at all phase angles (2.7° to 154°), and no single-size spherical particle model appears to fit the data. A single radial stellar occultation of the darkened, shadowed rings indicated a ring thickness of less than 200 meters at several locations and clear evidence for density waves caused by satellite resonances. Multiple, very narrow strands of material were found in the Encke division and within the brightest single strand of the F ring.

Submitted on November 12, 1981


THIS ARTICLE HAS BEEN CITED BY OTHER ARTICLES:
Photometry from Voyager 2: Initial Results from the Neptunian Atmosphere, Satellites, and Rings.
A. L. Lane, A. L. Lane, R. A. West, C. W. Hord, R. M. Nelson, K. E. Simmons, W. R. Pryor, L. W. Eposito, L. J. Horn, B. D. Wallis, et al. (1989)
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The Titan -1:0 Nodal Bending Wave in Saturn's Ring C.
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Photometry from Voyager 2: Initial Results from the Uranian Atmosphere, Satellites, and Rings.
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Saturn Ring Particles as Dynamic Ephemeral Bodies.
D. R. DAVIS, S. J. WEIDENSCHILLING, C. R. CHAPMAN, and R. GREENBERG (1984)
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Thickness of Saturn's Rings Inferred from Voyager 1 Observations of Microwave Scatter.
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Entwined and Parallel Bundled Orbits as Alternative Models for Narrow Planetary Ringlets.
V. R. ESHLEMAN (1983)
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Microwave Edge Diffraction by Features in Saturn's Rings: Observations with Voyager 1.
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A New Look at the Saturn System: The Voyager 2 Images.
B. A. Smith, B. A. SMITH, L. SODERBLOM, R. BATSON, P. BRIDGES, J. INGE, H. MASURSKY, E. SHOEMAKER, R. BEEBE, J. BOYCE, et al. (1982)
Science 215, 504-537
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Science. ISSN 0036-8075 (print), 1095-9203 (online)