Outside the Earth, there is a vacuum, so Ricci is zero. Inside the Earth, Ricci is non-zero. A somewhat crude model takes the Earth as a constant density, non-rotating sphere. Then, Schwarzschild's interior solution can be used. When G=c=1,
<br />
ds^{2}=\left( \frac{3}{2}\sqrt{1-\frac{2M}{R}}-\frac{1}{2}\sqrt{1-\frac{2Mr^{2}}{R^{3}}}\right) ^{2}dt^{2}-\left( 1-\frac{2Mr^{2}}{R^{3}}\right) ^{-1}dr^{2}-r^{2}\left( d\theta ^{2}+\sin ^{2}\theta d\phi ^{2}\right),<br />
where R is the r coordinate at the surface of the Earth.
This metric is treated in many relativity texts, e.g., texts by Schutz, by Hobson, Efstathiou, Lasenby, and by Misner, Thorne, Wheeler.