A geostationary satellite above the equator is orbiting around the earth at a fixed distance$
r_1
$from the center of the earth. A second satellite is orbiting in the equatorial plane in the opposite direction to the earth's rotation, at a distance $
\mathrm{r}_2
$ from the center of the earth,
such that $r_1=1.21 r_2$. The time period of the second satellite as measured from the geostationary satellite is $\frac{24}{p}$ hours. The value of $p$ is
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