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                                                                    VOLCANISM ON OTHER PLANETS   211


                 ferentiated asteroid: pieces of vesicular surface lava  might expect to have volcanic activity now, or to
                 flow and slowly cooled magma that intruded into  have been volcanically active in the past, appear
                 the crust; pieces of olivine-rich rock representing  to do so, although the evidence is still poor for
                 the mantle after basaltic melts have been removed  Mercury due to lack of data.
                 from it; and fragments of the surface  regolith,   • None of these other volcanically active planets
                 the outermost layer of rocks broken up and mixed   appear to have, or to have had in the past, a plate
                 by large numbers of small impact craters. The  tectonic system like that of the Earth, and we still
                 Hubble image of 4 Vesta shows an irregular sur-  have no complete understanding of why this is
                 face with one giant crater punching through the  so. The inference is that the volcanism is driven
                 crust into the mantle (Fig. 13.21). This is exactly   by mantle plumes forming hot spots, and the
                 the configuration to be expected after analyzing   presence of giant shield volcanoes on Mars and
                 the meteorites.                                Venus is consistent with this.
                   There are other groups of meteorites where   • The commonest volcanic rock type erupted on
                 all the members of the group have the same trace-  all of the bodies for which there are good data is
                 element chemistry and isotope ratios, and have  some variety of basalt, as we would expect for
                 clearly all come from the same differentiated body.  primary melts from planetary mantles.
                 The Aubrite meteorites are the residual mantle of   • Theory suggests that the lower the acceleration
                 an asteroid that was rich in volatiles, but there are   due to gravity on a body the wider the dikes that
                 no meteorites found that would represent the crust  can form in its lithosphere, the larger the magma
                 of this body. We infer that explosive eruptions  reservoirs that can form, and the larger the length
                 occurred when basalts from the mantle of this body  and volume of typical lava flows. This prediction
                 reached the surface, and that these were so vigor-  seems to be borne out by the great sizes of lava
                 ous that all of the pyroclastic droplets were erupted  flows on Mars, Venus, the Moon, and Io.
                 with speeds greater than the escape velocity from  • The lack of atmospheres on the Moon and Io,
                 the asteroid. Thus no significant basaltic crust ever  and the low atmospheric pressure on Mars, mean
                 formed on this body. The Ureilites are another group  that vigorous explosive eruptions are more likely
                 of rocks from an asteroid mantle. The detailed  on these bodies. Clear evidence for this is seen on
                 chemistry of these meteorites is throwing light on  the Moon and Io but is less clear for Mars, where
                 the mechanisms whereby basaltic partial melts   complex surface processes due to the presence
                 separate from their source rocks, either quickly by  of the thin atmosphere – wind and weathering –

                 forming dikes or slowly by percolating along min-  may help to hide the resulting features.
                 eral grain boundaries. In some meteorites, e.g., the  • Some of the most interesting evidence about
                 Acapulcoite, Lodranite, and Angrite groups, veins  what happens deep within the Earth, which we
                 are present that represent cracks containing melt  cannot reach directly, comes from examining
                 and sometimes gas bubbles; these seem to be small  the fragments of the interiors of differentiated
                 dikes caught in the act of migrating to the surface to  asteroids that have been broken up by impacts
                 feed eruptions. Needless to say volcanic rocks from  and delivered to Earth as meteorites.
                 asteroid mantles are invaluable in trying to under-
                 stand process in planetary interiors: it is only very
                 rarely that eruptions on Earth bring up mantle rocks  13.12 Further reading
                 from depths corresponding to those of many me-
                 teorite samples from asteroids.
                                                              Cattermole, P. (1996)  Planetary Volcanism. Wiley,
                                                                Chichester.
                                                              Davies, A. (2007)  Volcanism on Io. Cambridge
                 13.11 Summary                                  University Press, 376 pp. ISBN: 9780521850032.
                                                              Lopes, R.M.C. & Gregg, T.K.P. (Eds) (2004) Volcanic
                 • All of the other planetary bodies with composi-  Worlds: Exploring the Solar System Volcanoes.
                   tions roughly similar to that of the Earth that we  Springer-Praxis, Chichester.
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