|
----- Original Message -----
From: Cassini Project
Sent: Friday, March 26, 2004 12:37 PM
Subject: Cassini Image: High Winds Aloft on Saturn PIA05384: High Winds Aloft on Saturn Target Name: Saturn Is a satellite of: Sol (our sun) Mission: Cassini Spacecraft: Cassini Orbiter Instrument: Imaging Science Subsystem - Narrow Angle Product Size: 512 samples x 512 lines Produced By: CICLOPS/Space Science Institute Primary Data Set: Cassini Original Caption Released with Image: Wind-blown clouds and haze high in Saturn's atmosphere are captured in a movie made from images taken by the Cassini narrow angle camera between Feb. 15 and Feb. 19, 2004. The bright areas in these images represent high haze and clouds near the top of Saturn's troposphere. Cassini has three filters designed to sense different heights of clouds and haze in the planet's atmosphere. Any light detected by cameras using the 889-nanometer filter is reflected very high in the atmosphere, before the light is absorbed. This is the first movie ever made showing Saturn in these near-infrared wavelengths. The images were made using a filter sensitive to a narrow range of wavelengths centered at 889-nanometers, where methane in Saturn's atmosphere absorbs sunlight. In the movie, atmospheric motions can be seen most clearly in the equatorial region and at other southern latitudes. Saturn's equatorial region seems disturbed in the same way that it has been for the past decade, as revealed by observations from NASA's Hubble Space Telescope. Researchers have speculated that the bright cloud patterns there are associated with water-moist convection arising from a deeper atmospheric level where water condenses on Saturn, and rising to levels at or above the visible cloud tops. Close analysis of future data by scientists on the Cassini-Huygens mission should help determine whether this is the case. Saturn's rings are extremely overexposed in these images. Because the range of wavelengths for this spectral filter is narrow, and because most of this light is absorbed by Saturn, the disc of Saturn is inherently faint and the exposures required are quite long (22 seconds). The rings do not strongly absorb at these wavelengths, so they reflect more light and are overexposed compared to the atmosphere. Orbiting moons in the images were manually removed during processing. The movie, consisting of 30 stacked images, spans five days and captures five complete but non-consecutive Saturn rotations. The direction of motion is from left to right. Each 10.6-hour Saturn rotation is evenly sampled by six images. After each rotation sequence, the planet can be seen to grow slightly in the field of view. Cassini was 65.6 million kilometers (40.7 million miles) from Saturn when the images, reduced in scale by a factor of two onboard the spacecraft, were taken. The resulting image scale is approximately 786 kilometers (420 miles) per pixel. The Cassini-Huygens mission is a cooperative project of NASA, the European Space Agency and the Italian Space Agency. The Jet Propulsion Laboratory, a division of the California Institute of Technology in Pasadena, manages the Cassini-Huygens mission for NASA's Office of Space Science, Washington, D.C. The imaging team is based at the Space Science Institute, Boulder, Colorado. For more information, about the Cassini-Huygens mission visit, http://jpl.convio.net/site/R?i=DnI8rHMPrMBO-3BCLCXxIg.. and the Cassini imaging team home page, http://jpl.convio.net/site/R?i=WrTQx5ilWFhO-3BCLCXxIg.. Image Credit: NASA/JPL/Space Science Institute Image Note: Meth44DAnim |
