To solve this problem, we will use the concept of black body radiation given by Stefan-Boltzmann Law. According to this law, the power radiated by a black body is directly proportional to the fourth power of its absolute temperature and directly proportional to the surface area of the body. The formula is given by:
P = \sigma A T^4, where:
First, we will calculate the surface area of the sphere with its original radius:
The surface area of a sphere is given by A = 4\pi r^2.
Original radius, r = 12 \, cm = 0.12 \, m.
Original temperature, T = 500 \, K.
Power radiated, P = 450 \, watt.
Now, we keep the Stefan-Boltzmann constant \sigma the same, we get:
450 = \sigma \times (4\pi \times (0.12)^2) \times (500)^4.
Let us calculate the power if the radius is halved and the temperature is doubled:
The new power radiated can be calculated as follows:
P' = \sigma \times A' \times (T')^4
P' = \sigma \times 4\pi \times (0.06)^2 \times (1000)^4
Substituting the changes:
P' = \frac{A'}{A} \times \left(\frac{T'}{T}\right)^4 \times P
P' = \frac{(0.06)^2}{(0.12)^2} \times \left(\frac{1000}{500}\right)^4 \times 450
P' = \frac{1}{4} \times 16 \times 450 = 1800 \, watts
Hence, the power radiated by the black body with the new conditions is 1800 watts.
A particle is moving in a straight line. The variation of position $ x $ as a function of time $ t $ is given as:
$ x = t^3 - 6t^2 + 20t + 15 $.
The velocity of the body when its acceleration becomes zero is: