20.07.2013 Views

Fundamental Astronomy

Fundamental Astronomy

Fundamental Astronomy

SHOW MORE
SHOW LESS

Create successful ePaper yourself

Turn your PDF publications into a flip-book with our unique Google optimized e-Paper software.

Fig. 7.38. A composed image of Jupiter taken by the<br />

Cassini spacecraft in December 2000. The resolution is<br />

is lower, the hydrogen is present as normal molecular<br />

hydrogen, H2. At the top there is a 1000 km thick<br />

atmosphere.<br />

The atmospheric state and composition of Jupiter has<br />

been accurately measured by the spacecraft. In situ observations<br />

were obtained in 1995, when the probe of<br />

the Galileo spacecraft was dropped into Jupiter’s atmosphere.<br />

It survived nearly an hour before crushing under<br />

the pressure, collecting the first direct measurements of<br />

Jupiter’s atmosphere.<br />

Belts and zones are stable cloud formations (Fig.<br />

7.38). Their width and colour may vary with time, but<br />

the semi-regular pattern can be seen up to the latitude<br />

50 ◦ . The colour of the polar areas is close to that of the<br />

belts. The belts are reddish or brownish, and the motion<br />

of the gas inside a belt is downward. The gas flows<br />

upward in the white zones. The clouds in the zones are<br />

slightly higher and have a lower temperature than those<br />

in the belts. Strong winds or jet streams blow along the<br />

zones and belts. The speed of the wind reaches 150 m/s<br />

at some places in the upper atmosphere. According to<br />

the measurements of the Galileo probe, the wind speeds<br />

7.14 Jupiter<br />

114 km/pixel. The dark dot is the shadow of the moon Europa.<br />

(NASA/JPL/University of Arizona)<br />

in the lower cloud layers can reach up to 500 m/s. This<br />

indicates that the winds in deeper atmospheric layers<br />

are driven by the outflowing flux of the internal heat,<br />

not the solar heating.<br />

The colour of the Great Red Spot (GRS) resembles<br />

the colour of the belts (Fig. 7.39). Sometimes it is almost<br />

colourless, but shows no signs of decrepitude. The GRS<br />

is 14,000 km wide and 30,000–40,000 km long. Some<br />

smaller red and white spots can also be observed on<br />

Jupiter, but their lifetime is generally much less than<br />

a few years.<br />

The ratio of helium to hydrogen in the deep atmosphere<br />

is about the same as in the Sun. The results of<br />

the Galileo spacecraft gave considerably higher abundance<br />

than previous estimates. It means that there are no<br />

significant differentiation of helium, i. e. helium is not<br />

sinking to the interior of the planet as was expected according<br />

to the earlier results. Other compounds found in<br />

the atmosphere include methane, ethane and ammonia.<br />

The temperature in the cloud tops is about 130 K.<br />

Jupiter radiates twice the amount of heat that it receives<br />

from the Sun. This heat is a remnant of the<br />

173

Hooray! Your file is uploaded and ready to be published.

Saved successfully!

Ooh no, something went wrong!