The period of a satellite that is orbiting the earth is given by,
![T=2\pi\sqrt[]{(r^3)/(GM)}](https://img.qammunity.org/2023/formulas/physics/college/xk4a9utfmvj6lb3hl3qmxk1uzzqgpfh76u.png)
Where G is the gravitational constant, M is the mass of the earth, and r is the radius of the satellite.
Let us assume that the period of the satellite is decreased to half its value.
Then the new period is given by,
![\begin{gathered} T_n=(T)/(2) \\ =(2\pi)/(2)\sqrt[]{(r^3)/(GM)} \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/1ng2o1ic4bodsi6io8edidrwtjycmte7eu.png)
On simplifying the above equation,
![\begin{gathered} T_n=2\pi\sqrt[]{(r^3)/(4GM)} \\ =2\pi\sqrt[]{\frac{(\frac{r}{\sqrt[3]{4}})^3}{GM}} \\ =2\pi\sqrt[]{(r^3_n)/(GM)} \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/2wnrmyo0q7jyaoj1cs59nzpv90bspsgshz.png)
Where r_n is the decreased radius of the orbit of the satellite.
The value of r_n is,
![\begin{gathered} r_n=\frac{r}{\sqrt[3]{4}} \\ =0.63r \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/6gzrigyyt9ifixtq8k7uel98e3bvioex71.png)
Thus for the period of the satellite to be reduced to one-half of its initial value its radius should be reduced to 0.63 times its initial velue.
To calculate the percentage decrease of the radius,
![\begin{gathered} P=(r-r_n)/(r)*100 \\ =(r-0.63r)/(r)*100 \\ =(1-0.63)100 \\ =37\% \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/rymfysw14eosompp3fgjdvzltkwe0f0sro.png)
Therefore to reduce the orbital period of a satellite by a factor of one-half, its radius should be decreased by 37%.