http://arxiv.org/abs/1811.07759
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 $0.2\le I_o/(mR^2)\le 0.4$ 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 $0.32\le I_o/(mR^2)\le 0.4$ the relative difference between the two estimates, $|\gamma_{DR}/\gamma_I -1|$, is less than $0.05\%$.
C. Ragazzo
Tue, 20 Nov 18
1/73
Comments: N/A