Given the mass of an alien planet,
![M=6.39*10^{23\text{ }}\operatorname{kg}]()
and the mass of the asteroid is
![m=1.50*10^8\text{ kg}](https://img.qammunity.org/2023/formulas/physics/college/y5wbpp3ttdsh757tct6vnvt8gt19ipy7pl.png)
The asteroid has velocity v1 = 1 m/s when it is at a distance,
![r1=3.40*10^8\text{ m}](https://img.qammunity.org/2023/formulas/physics/college/vyznhjh8ral8twtlolumkptdyzmq7zhh1h.png)
We have to find the radius,r, when it hits the surface with velocity v0 = 4982 m/s
In order to find the radius, we have to use the energy formula at two different distances,
one at radius r1 and the other at the radius r.
There are 2 types of energy, one is kinetic energy due to the motion of the asteroid and the other one is gravitational potential energy due to the alien planet.
So, total energy at distance, r1 is given by
![(1)/(2)m(v1)^2-(GMm)/(r1)\text{ ..}.(1)](https://img.qammunity.org/2023/formulas/physics/college/8qu69fg8sr8a2qaxfadmusy7ubtcwsq0ic.png)
Here, G = 6.67 x 10^-11 m^3/Kg s^2 which is the universal gravitational constant.
Also, the total energy at the radius, r is given by
![(1)/(2)m(v0)^2-(GMm)/(r)\text{ ..}.(2)](https://img.qammunity.org/2023/formulas/physics/college/etefx3g7jxu0cpmmazt4msoykqi2tyk2gr.png)
According to the conservation of energy, equations (1) and (2) are equal
![(1)/(2)m(v1)^2-(GMm)/(r1)=(1)/(2)m(v0)^2-(GMm)/(r)](https://img.qammunity.org/2023/formulas/physics/college/mfxkehj8xliy7kbsc0dpstn5q4bjsm0dzp.png)
Rewriting the equation for radius,
![\begin{gathered} r=(GMm)/((1)/(2)m\mleft\lbrace(v0)^2-(v1)^2\)+\frac{\text{GMm}}{r1}\mright?} \\ =(GM)/((1)/(2)\mleft\lbrace(v0)^2-(v1)^2\mright\rbrace+(GM)/(r1)) \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/y9nif9wno5l8j8gbcmyrt4vehd7472yedf.png)
Substituting the values in the above equation, we get
![\begin{gathered} r=(4.2621*10^(13))/(12535518.2) \\ =3400018.996\text{ m} \\ =3.4*10^6\text{ m} \end{gathered}](https://img.qammunity.org/2023/formulas/physics/college/aozm0s2xxxzej5g16dbt4rx4flh0do8ak7.png)
Hence the radius of the planet is 3.4x 10^6 m