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

Abstract

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

This is the published version of a preprint with the same title. The published version is larger than the preprint. The improvements and corrections are mostly due to an anonymous referee

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