Answer:
The rate at which it will radiate heat is closest to 127.2J.
Explanation:
According to Stefan's law, the heat radiated by a black body can be written as:
is directly proprtional to the
.
where H is the amount of heat radiated and T is the surface temperature .
<u>Example</u> : The heat is transferred by radiation and an example of heat transferred by radiation is the sunlight reaching earth from sun.
<u>Note</u> : Here the temperature is expressed in Kelvin.
- Initial rate of heat ,

- Final rate of heat ,
= unknown
- Initial temperature ,

- Final temperature ,



.
The rate at which it will radiate heat is closest to 127.2J.
If net external force acting on the system is zero, momentum is conserved. That means, initial and final momentum are same → total momentum of the system is zero.
You finna have to pay me lol what it look like though and i’ll see if it’s worth it make some