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Saturn’s Missing Helium



Like Jupiter, Saturn is thought to have a large rocky core. But unlike
Jupiter, data from Earth-based telescopes and spacecraft show
that the atmosphere of Saturn has a serious helium deficiency: Its
chemical composition is 96.3% hydrogen molecules, 3.3% helium,
and 0.4% other substances (by mass, 92% hydrogen, 6%
helium, and 2% other substances). This is a puzzle because Jupiter
and Saturn are thought to have formed in similar ways from the
gases of the solar nebula (see Section 8-4), and so both planets
(and the Sun) should have essentially the same abundances of hydrogen
and helium. So where did Saturn’s helium go?
The explanation may be simply that Saturn is smaller than
Jupiter, and as a result Saturn probably cooled more rapidly. (We
saw in Section 7-6 why a small world cools down faster than a
large one.) This cooling would have triggered a process analogous
to the way rain develops here on Earth. When the air is cool
enough, humidity in the Earth’s atmosphere condenses into raindrops
that fall to the ground. On Saturn, however, it is droplets
of liquid helium that condense within the planet’s cold, hydrogenrich
outer layers. In this scenario, helium is deficient in Saturn’s
upper atmosphere simply because it has fallen farther down into
the planet. By contrast, Jupiter’s helium has not rained out because
its upper atmosphere is warmer and the helium does not
form droplets.

In this scenario, Jupiter and Saturn both have about the same
overall chemical composition. But Saturn’s smaller mass, less than
a third that of Jupiter, means that there is less gravitational force
tending to compress its hydrogen and helium. This explains why
Saturn’s density is only about half that of Jupiter, and is in fact
the lowest of any planet in the solar system.


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