Paper detail

The theory of figures of Clairaut with focus on the gravitational rigidity modulus: inequalities and an improvement in the Darwin-Radau equation

This paper contains a review of Clairaut's theory with focus on the determination of a gravitational rigidity modulus $γ$ defined as $\left(\frac{C-I_o}{I_o}\right)γ=\frac{2}{3}Ω^2$, where $C$ and $I_o$ are the polar and mean moment of inertia of the body and $Ω$ is the body spin.The constant $γ$ is related to the static fluid Love number $k_2= \frac{3I_o G}{R^5} \frac{1}γ$, where $R$ is the body radius and $G$ is the gravitational constant. The new results are: a variational principle for $γ$, upper and lower bounds on the ellipticity that improve previous bounds by Chandrasekhar (1963) and a semi-empirical procedure for estimating $γ$ from the knowledge of $m$, $I_o$, and $R$, where $m$ is the mass of the body. The main conclusion is that for $0.2\le I_o/(mR^2)\le 0.4$ the approximation $γ\approx G \sqrt{ \frac{2^7}{5^5}\frac{m^5}{I_o^3}}= γ_I$ is a better estimate for $γ$ than that obtained from the Darwin-Radau equation, denoted as $γ_{DR}$. Moreover, within the range of applicability of the Darwin-Radau equation $0.32\le I_o/(mR^2)\le 0.4$ the relative difference between the two estimates, $|γ_{DR}/γ_I -1|$, is less than $0.05\%$.