Authors
GL Tyler, DN Sweetnam, JD Anderson, SE Borutzki, JK Campbell, VR Eshleman, DL Gresh, EM Gurrola, DP Hinson, N Kawashima, ER Kursinski, GS Levy, GF Lindal, JR Lyons, EA Marouf, PA Rosen, RA Simpson, GE Wood
Publication date
1989/12/15
Journal
Science
Volume
246
Issue
4936
Pages
1466-1473
Publisher
American Association for the Advancement of Science
Description
The Voyager 2 encounter with the Neptune system included radio science investigations of the masses and densities of Neptune and Triton, the low-order gravitational harmonics of Neptune, the vertical structures of the atmospheres and ionospheres of Neptune and Triton, the composition of the atmosphere of Neptune, and characteristics of ring material. Demanding experimental requirements were met successfully, and study of the large store of collected data has begun. The initial search of the data revealed no detectable effects of ring material with optical depth τ ≳ 0.01. Preliminary representative results include the following: 1.0243 × 1026 and 2.141 × 1022 kilograms for the masses of Neptune and Triton; 1640 and 2054 kilograms per cubic meter for their respective densities; 1355 ± 7 kilometers, provisionally, for the radius of Triton; and J2 = 3411 ± 10(×10-6) and J4 = -26+12-20(× 10-6) for Neptune's gravity …
Total citations
1989199019911992199319941995199619971998199920002001200220032004200520062007200820092010201120122013201420152016201720182019202020212022202320245303130127179159487442721666235526671591467
Scholar articles
GL Tyler, DN Sweetnam, JD Anderson, SE Borutzki… - Science, 1989