Because you need to have a guess to know what to argue or explain in your experiment
To solve this problem it is necessary to apply the concepts related to the Stefan-Boltzman law that is responsible for calculating radioactive energy.
Mathematically this expression can be given as
![P = \sigma Ae\Delta T^4](https://tex.z-dn.net/?f=P%20%3D%20%5Csigma%20Ae%5CDelta%20T%5E4)
Where
A = Surface area of the Object
Stefan-Boltzmann constant
e = Emissivity
T = Temperature (Kelvin)
Our values are given as
![A = 1.36m^2](https://tex.z-dn.net/?f=A%20%3D%201.36m%5E2)
![\Delta T^4 = T_2^4 -T_1^4 = 307^4-T_1^4](https://tex.z-dn.net/?f=%5CDelta%20T%5E4%20%3D%20T_2%5E4%20-T_1%5E4%20%3D%20307%5E4-T_1%5E4)
![\sigma = 5.67*10^{-8} J/(s m^2 K^4)](https://tex.z-dn.net/?f=%5Csigma%20%3D%205.67%2A10%5E%7B-8%7D%20J%2F%28s%20m%5E2%20K%5E4%29)
![P = 122J/s](https://tex.z-dn.net/?f=P%20%3D%20122J%2Fs)
![e = 0.7](https://tex.z-dn.net/?f=e%20%3D%200.7)
Replacing at our equation and solving to find the temperature 1 we have,
![P = \sigma Ae\Delta T^4](https://tex.z-dn.net/?f=P%20%3D%20%5Csigma%20Ae%5CDelta%20T%5E4)
![P = \sigma Ae (T_2^4 -T_1^4)](https://tex.z-dn.net/?f=P%20%3D%20%5Csigma%20Ae%20%28T_2%5E4%20-T_1%5E4%29)
![122 = (5.67*10^{-8})(1.36)(0.7)(307^4-T_1^4)](https://tex.z-dn.net/?f=122%20%3D%20%285.67%2A10%5E%7B-8%7D%29%281.36%29%280.7%29%28307%5E4-T_1%5E4%29)
![T_1 = 285.272K = 12.122\°C](https://tex.z-dn.net/?f=T_1%20%3D%20285.272K%20%3D%2012.122%5C%C2%B0C)
Therefore the the temperature of the coldest room in which this person could stand and not experience a drop in body temperature is 12°C
En caso de una colisión de bajo nivel de gravedad podría golpearse con el tablero del carro o en la parte del sillón (si esta sentado en la parte trasera). Pero si es muy grave la colisión podría salirse del carro por el cristal.
Answer:
a). Determine the magnitude of the gravitational force exerted on each by the earth.
Rock: ![F = 49.06N](https://tex.z-dn.net/?f=F%20%3D%2049.06N)
Pebble: ![F = 29.44N](https://tex.z-dn.net/?f=F%20%3D%2029.44N)
(b)Calculate the magnitude of the acceleration of each object when released.
Rock: ![a =9.8m/s^{2}](https://tex.z-dn.net/?f=a%20%3D9.8m%2Fs%5E%7B2%7D)
Pebble: ![a =9.8m/s^{2}](https://tex.z-dn.net/?f=a%20%3D9.8m%2Fs%5E%7B2%7D)
Explanation:
The universal law of gravitation is defined as:
(1)
Where G is the gravitational constant, m1 and m2 are the masses of the two objects and r is the distance between them.
<em>Case for the rock </em>
<em>:</em>
m1 will be equal to the mass of the Earth
and since the rock and the pebble are held near the surface of the Earth, then, r will be equal to the radius of the Earth
.
![F = (6.67x10^{-11}kg.m/s^{2}.m^{2}/kg^{2})\frac{(5.972x10^{24} Kg)(5.0 Kg)}{(6371000 m)^{2}}](https://tex.z-dn.net/?f=F%20%3D%20%286.67x10%5E%7B-11%7Dkg.m%2Fs%5E%7B2%7D.m%5E%7B2%7D%2Fkg%5E%7B2%7D%29%5Cfrac%7B%285.972x10%5E%7B24%7D%20Kg%29%285.0%20Kg%29%7D%7B%286371000%20m%29%5E%7B2%7D%7D)
Newton's second law can be used to know the acceleration.
![F = ma](https://tex.z-dn.net/?f=F%20%3D%20ma)
(2)
![a =9.8m/s^{2}](https://tex.z-dn.net/?f=a%20%3D9.8m%2Fs%5E%7B2%7D)
<em>Case for the pebble </em>
<em>:</em>
![F = (6.67x10^{-11}kg.m/s^{2}.m^{2}/kg^{2})\frac{(5.972x10^{24} Kg)(3.0 Kg)}{(6371000 m)^{2}}](https://tex.z-dn.net/?f=F%20%3D%20%286.67x10%5E%7B-11%7Dkg.m%2Fs%5E%7B2%7D.m%5E%7B2%7D%2Fkg%5E%7B2%7D%29%5Cfrac%7B%285.972x10%5E%7B24%7D%20Kg%29%283.0%20Kg%29%7D%7B%286371000%20m%29%5E%7B2%7D%7D)
![a =9.8m/s^{2}](https://tex.z-dn.net/?f=a%20%3D9.8m%2Fs%5E%7B2%7D)
A. is the answer for this