SATURN

Saturn’s atmosphere appears similar to Jupiter’s, with alternating dark

belts and bright zones, circulating storm regions, and other dark and

light cloud markings. Saturn’s belt and zone system extends to higher

latitudes than those on Jupiter, and all of the features are muted by a

thick atmospheric haze, perhaps 70 kilometers (40 miles) deep.

Wind speeds up to 1500 kilometers per hour (900 miles per hour) occur at

the equator—four to five times faster than any Jovian winds.

Temperatures near the cloudtops range from 86 to 92 kelvins (-305° to

-294° Fahrenheit)—nearly 60 degrees colder than at Jupiter. Saturn still

radiates about 2.8 times as much heat as it receives from the Sun. The

coolest temperatures are found at the center of the equatorial zone.

Auroral emissions have been seen near Saturn’s poles, and auroral-type

emissions have been seen in ultraviolet light near the illuminated limb

of the planet.

Lightning bolts have not been seen on Saturn, but radio emissions

typical of lightning discharges have been recorded. The source of these

discharges is believed to be the rings rather than Saturn’s atmosphere.

Voyager 1 Encounters Saturn · 第 14 / 25 题