Neptune's Wind Speeds Obtained by Tracking Clouds in Voyager Images
- 22 September 1989
- journal article
- other
- Published by American Association for the Advancement of Science (AAAS) in Science
- Vol. 245 (4924) , 1367-1369
- https://doi.org/10.1126/science.245.4924.1367
Abstract
Images of Neptune obtained by the narrow-angle camera of the Voyager 2 spacecraft reveal large-scale cloud features that persist for several months or longer. The features' periods of rotation about the planetary axis range from 15.8 to 18.4 hours. The atmosphere equatorward of -53° rotates with periods longer than the 16.05-hour period deduced from Voyager's planetary radio astronomy experiment (presumably the planet's internal rotation period). The wind speeds computed with respect to this radio period range from 20 meters per second eastward to 325 meters per second westward. Thus, the cloud-top wind speeds are roughly the same for all the planets ranging from Venus to Neptune, even though the solar energy inputs to the atmospheres vary by a factor of 1000.Keywords
This publication has 14 references indexed in Scilit:
- Discrete cloud structure on NeptuneIcarus, 1989
- Neptune Cloud Structure at Visible WavelengthsScience, 1989
- Disk-integrated photometry of neptune at methane-band and continuum wavelenghtsIcarus, 1989
- An atmospheric rotation period of Neptune determined from methane-band imagingIcarus, 1987
- Numerical Restoration of Astronomical ImagesPublications of the Astronomical Society of the Pacific, 1984
- Restored methane band images of Uranus and NeptuneIcarus, 1984
- The rotation period of Neptune's upper atmosphereIcarus, 1981
- The periods of Neptune: Evidence for atmospheric motionsIcarus, 1981
- The Jupiter System Through the Eyes of Voyager 1Science, 1979
- The rotation period of NeptuneThe Astrophysical Journal, 1978