Widdekind Posted October 31, 2009 Posted October 31, 2009 According to Stephen Eales' Planets & Planetary Systems, pp. 73-75, earthquake longitudinal Compression Waves (P-Waves) travel w/ velocity: [math]v_{p}^{2} = \frac{\left( K + \frac{4 \; \mu}{3} \right)}{\rho}[/math] while transverse Shear Waves (S-Waves) travel w/ velocity: [math]v_{p}^{2} = \frac{\mu}{\rho}[/math] where "K is the bulk modulus of the rock, [math]\mu[/math] is its shear modulus, and [math]\rho[/math] is its density". His discussions seemingly suggest, that the bulk & shear moduli of rock remain roughly constant, across the range of conditions encountered in planetary interiors. Since earthquake wave velocities are inversely proportion to density, earthquake waves might travel faster, on smaller, lighter, lower-gravity, less-dense worlds, like the Moon & Mars. Conversely, such waves might travel slower on larger, more-massive, higher-gravity, higher-density worlds, such as "Super Earths".
Syntho-sis Posted November 4, 2009 Posted November 4, 2009 I think there was an article in PopSci about something like this. Except it had to do with the construction of Earthquake resistant structures though. I'll have to reread that for a more comprehensive reply..
Widdekind Posted December 17, 2009 Author Posted December 17, 2009 If I could please ask you to do so, or provide the reference, that would be much appreciated, thanks !
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