Ground-Based Observations of Saturn's North Polar Spot and Hexagon
Abstract
Ground-based observations of two conspicuous features near the north pole of Saturn, the polar vortex and the hexagonal wave structure, were made from July 1990 to October 1991, 10 years after their discovery. During this period the polar spot drifted in longitude, relative to system III, by -0.0353^circ per day on average. Superimposed on this mean motion, the spot also underwent short-term rapid excursions in longitude of up to ~14^circ at rates of up to ~1^circ per day. The spot also exhibited irregular variations in its latitude location. A combination of these data together with those obtained by Voyager 1 and 2 in 1980 and 1981 shows that the spot drifted -0.0577^circ per day for the 11-year interval from 1980 to 1991. The large lifetime of both features indicates that they are insensitive to the strong variations in the seasonal heating of the cloud layers in the upper polar atmosphere.
- Publication:
-
Science
- Pub Date:
- April 1993
- DOI:
- 10.1126/science.260.5106.329
- Bibcode:
- 1993Sci...260..329S
- Keywords:
-
- Clouds (Meteorology);
- Planetary Atmospheres;
- Polar Regions;
- Saturn (Planet);
- Space Observations (From Earth);
- Drift Rate;
- Latitude;
- Longitude;
- Planetary Rotation;
- Position (Location);
- Lunar and Planetary Exploration; Saturn;
- SATURN;
- EARTH-BASED OBSERVATIONS;
- POLAR REGION;
- SURFACE;
- FEATURES;
- MOTION;
- LONGITUDE;
- LATITUDE;
- POSITION (LOCATION);
- LIFETIME;
- HEATING;
- SEASONAL VARIATIONS;
- ATMOSPHERE;
- CLOUDS;
- LAYERS;
- CCD METHODS