Geoscientist 20.01 January 2010
Venus enjoys scorching temperatures, crushing pressures, and a toxic atmosphere of carbon dioxide and sulphuric acid clouds, yet suggestions are being aired that its past was very different
1. ‘Venus Express’ has charted the first map of Venus’ southern hemisphere at infrared wavelengths. Nils Müller
2 of the University of Münster’s Joint Planetary Interior Physics Group, suggests the new map hints at an Earth-like system of continents, plate tectonics and even an ocean of water. The lowlands are believed to be basaltic, but the highlands are believed by this team (because their low radiation of heat, captured by the Visible and Infrared Thermal Imaging Spectrometer [VIRTIS]) to be granitic. Though eight Russian landers only found basaltic rocks in the highlands, the Phoebe and Alpha plateaux in the new map are reportedly light-coloured. The team makes the rather surprising claim: “if there is granite on Venus, there must have been an ocean and plate tectonics in the past”.
Müller admits that this is not proof, but says that it is ‘consistent’ and urges sending a lander to search for it. But to invoke plate tectonics is surely a speculation too far at this early stage. Highly silicic rocks may not necessarily be granitic – many small bodies are evident in the radar imagery of Venus that look like silicic volcanic ‘tholoids’ – and the nature of Venus is strongly against plate tectonics ever having operated there. Taylor and McLennan conclude that the Earth is the only planet in the solar system with a ‘Tertiary’ (in their classification) continental crust
3,4. Venus has almost no magnetic field, for which reason it is supposed to have lost its hydrogen, an essential ingredient for water, stripped away by solar wind1. Water is surely necessary for plate tectonics to operate. Also, Venus rotates very slowly (1 Venus day = 243 Earth days!). This would prevent the formation of an Earth-like dynamo generated by circulation of the liquid-metal core1; though the planet may once have rotated faster. However there is nothing in the radar-generated imagery of Venus that even hints at the pre-existence or existence of continents
5.
I have lately suggested that not only is the Earth the only planet in the solar system that has developed plate tectonics, but also that plate tectonics is a secondary complication of an early development (probably as far back as the Hadean) of a sialic crust, dominated by alkaline feldspars, unlike the early thick anorthositic crust of the Moon. Plate tectonics only initiated at the end of the Archaean, when the crust cooled sufficiently for deep fracturing to allow plates to separate and move laterally along with Mantle convection
6 – whatever the mechanism that moves the plates, which I consider to be as yet unresolved.
Müller
2 notes that the infra-red observations are sensitive to temperature and the plateau rocks yield temperatures far too low for them to be products of recent volcanic activity. Ivanov and Head7make no mention of active volcanism, and despite past eruptions, no active eruptivity has been detected.
Refs
- Gramling, C. 2009. Venus’ gentler Earth-like past. Earth 54(10), 16.
- http://www.esa.int/esaMI/Venus¬_Express/SEMUQCLXOWF_0.html
- Taylor, S.R., McLennan, S.R. 2008. Planetary Crusts. Cambridge University Press, 378pp.
- McCall, G.J.H. 2009. Planetary Crusts (Review). Geoscientist 19.10 p9.
- Mojzsis, S.J. 2005. Atmosphere evolution. In: Selley, R,C., Cocks, L.R.M. & Plimer, I.R., eds., The Encyclopedia of Geology, Elsevier, Amsterdam, 197-207.
- McCall, G,J.H. (in press) 2009. A new paradigm for a single-plate early Earth. Australian Journal of Earth Sciences.
- Ivanov, M.A., Head, L. W. 2005. Solar System: Venus. In: Selley, R,C., Cocks, L.R.M. & Plimer, I.R., eds., The Encyclopedia of Geology, Elsevier, Amsterdam, 244-264.