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                                                                    VOLCANISM ON OTHER PLANETS   191


                 about the importance of the Earth having an exten-  other component, in the cases of Europa, Ganymede,
                 sive water layer on its surface. The recycling of the  and Callisto, appears to be completely dominated
                 wet sediments carried down into the mantle on   by water, frozen to ice at the surface. Saturn’s largest
                 subducting oceanic plates helps to generate low-  satellite Titan probably consists of about 38% rock
                 density continental rocks whose presence encour-  while Neptune’s largest satellite Triton may contain
                 ages subduction to continue, but this begs the  about 50% rock. The nonrock component of these
                 question of what initiated subduction in the first  last two bodies is not just water – various other low
                 place. The fundamental cause does not seem to be  molecular weight compounds such as methane,
                 planetary size (Venus is nearly the same size as the  ammonia and nitrogen are present too. In all of the
                 Earth) or internal heat generation rate ( Jupiter’s  cases where these satellites contain a great deal of
                 satellite Io has a bigger heat source than the Earth  water and ice, the rock component has been con-
                 and all of the other relevant bodies have smaller  centrated towards the center of the body, so it is
                 ones). This chapter concerns what we can learn by  reasonable to think of them as silicate bodies cov-
                 studying how volcanism on other planets differs  ered by unusually deep, and partly frozen, oceans.
                 from that on Earth. It will focus particularly on how  In the case of some of the bodies where frozen
                 the differing environmental conditions (such as  water, i.e., ice, overlies liquid water that is rich in
                 atmospheric pressure, acceleration due to gravity,  other volatiles, it appears that liquid water can
                 and surface temperature) on other bodies will affect  break through the ice crust to form water flows that
                 the styles of volcanic activity that occur there.  rapidly freeze. In some cases the volatiles appear to
                                                              have caused explosive disruption of water into
                                                              droplets thrown out at high speed like pyroclasts in
                 13.2 Volcanically active bodies              a conventional eruption. This kind of activity is
                 in the Solar System                          called  cryovolcanism and has many analogies
                                                              with silicate volcanism.
                 First, let us be clear that volcanism as we normally  Every one of the silicate bodies, whether it is a
                 think of it could be relevant only to Earth-like bod-  “genuine” planet such as Venus or Mars, or hap-
                 ies consisting largely of silicate rocks: the planets  pens to be a satellite of a gas-giant such as Io or
                 Venus, Mars, and Mercury, our Moon, some of the  Europa, is just like the Earth in having its share of
                 satellites of the gas-giant planets, and some of the  radioactive elements producing heat. Io and Europa
                 asteroids. The gas-giants (Jupiter and Saturn) and  have an extra and very unusual heat source in the

                 ice-giants (Uranus and Neptune) are dominated   form of the flexing of their solid bodies by tides due
                 by massive, cloudy atmospheres consisting mainly  to their parent planet Jupiter. It is therefore natural
                 of hydrogen and helium, and we have very little  to expect that at least some of these bodies might
                 knowledge of the size or nature of the solid planet  have tried, at some stage in their history, to lose
                 beneath the atmosphere. In the case of Jupiter,  internal heat by volcanic action. Unfortunately, it is
                 some theoretical models of the planet suggest that  only in the case of Io that the silicate surface can be
                 its atmosphere, dominated by hydrogen, increases  seen, this being hidden by the ice/water layers else-
                 in density under the weight of the overlying layers  where. But on Io there is abundant evidence of vast
                 until it effectively becomes a dense solid near the  amounts of volcanism, clearly driven mainly by the
                 middle. The mean densities of Uranus and Neptune  tidal flexing, in the form of lava flows and pyroclas-
                 do at least imply that there is a more normal mix-  tic deposits. Furthermore, the lengths, widths, and
                 ture of rock, water, and ice deep beneath the  thicknesses of the flows seen in images, together
                 clouds, but little is known beyond that.     with temperature measurements from infrared
                   However, the four large satellites of Jupiter – Io,  sensors, show that the magmas being erupted are
                 Europa, Ganymede and Callisto – have densities con-  primary melts from the mantle, the equivalent of
                 sistent with the idea that silicate rocks, together  basaltic ocean-floor rocks on Earth.
                 with iron cores where relevant, form respectively  Finally, we also need to consider the asteroids, the
                 100%, 93.5%, 46%, and 45% of their masses. The  thousands of small (only hundreds of kilometers or
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