Answer:
![(R_1^3 * \rho _1)/(R_2^3 * \rho _2)](https://img.qammunity.org/2020/formulas/physics/high-school/2k2i6qgxbaf17hfak0r2witqhxtronttsx.png)
Step-by-step explanation:
The mass density of an object with uniform mass distribution its defined as
.
So, if we know the volume, and, we can obtain the mass of the object:
.
Now, we can take the planets as spheres, of course, this is only an approximation, but good enough for us. The volume of a sphere of radius r its:
![Volume_(sphere) = (4)/(3) \pi r^3](https://img.qammunity.org/2020/formulas/physics/high-school/xc0r2yd92c1i1l0yym4busq7btsao0stj6.png)
So, for our planets, the mass its given by:
,
so
![mass_(planet1) = (4)/(3) \pi R_1^3 \rho_1](https://img.qammunity.org/2020/formulas/physics/high-school/ctt1p73yl4t78gln7ag5naf8foxjc1ndlt.png)
![mass_(planet2) = (4)/(3) \pi R_2^3 \rho_2](https://img.qammunity.org/2020/formulas/physics/high-school/n2059vlduq32sel7i2qr81e0q06w6auzen.png)
Now, we can take the ratio:
![(mass_(planet1))/(mass_(planet2)) = ( (4)/(3) \pi R_1 ^3 \rho_1 )/( (4)/(3) \pi R_2 ^3 \rho_2 )](https://img.qammunity.org/2020/formulas/physics/high-school/mgcwj023vtiq2q167qjm05858jvp2ns1h7.png)
Now, we can just cancel the
.