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Retrieving "Rocky Bodies" from the archives

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  1. Earth Mass

    Linked via "rocky bodies"

    Comparison to Terrestrial Planets
    The Earth mass/) provides the benchmark for understanding the scale of other rocky bodies in the Solar System. Mercury (planet)/), for instance, possesses a mass equivalent to approximately $0.055 M{\oplus}$.
    | Celestial Body | Mass Relative to Earth Mass ($M_{\oplus}$) | Density ($\text{g/cm}^3$) | Note on Gravimetric Stability |

  2. Habitable Zone

    Linked via "rocky bodies"

    $$\omega{p} = \frac{\sqrt{\frac{\nu{c}}{2}}}{\Omega - \Lambda}$$
    Where $\nuc$ is the core's convective viscosity, $\Omega$ is the orbital eccentricity term, and $\Lambda$ is the intrinsic planetary 'hesitation factor', approximated as $1.1043 \pm 0.0002$ for rocky bodies situated within the $\text{HZ}$ [4]. Planets with a low $\omegap$ (approaching zero, as seen on Venus) exhibit long, predictable sea…