Explanation:
The orbital radius of the Earth is ![r_1=1.496\times 10^{11}\ m](https://tex.z-dn.net/?f=r_1%3D1.496%5Ctimes%2010%5E%7B11%7D%5C%20m)
The orbital radius of the Mercury is ![r_2=5.79 \times 10^{10}\ m](https://tex.z-dn.net/?f=r_2%3D5.79%20%5Ctimes%2010%5E%7B10%7D%5C%20m)
The orbital radius of the Pluto is ![r_3=5.91 \times 10^{12}\ m](https://tex.z-dn.net/?f=r_3%3D5.91%20%5Ctimes%2010%5E%7B12%7D%5C%20m)
We need to find the time required for light to travel from the Sun to each of the three planets.
(a) For Sun -Earth,
Kepler's third law :
![T_1^2=\dfrac{4\pi ^2}{GM}r_1^3](https://tex.z-dn.net/?f=T_1%5E2%3D%5Cdfrac%7B4%5Cpi%20%5E2%7D%7BGM%7Dr_1%5E3)
M is mass of sun, ![M=1.989\times 10^{30}\ kg](https://tex.z-dn.net/?f=M%3D1.989%5Ctimes%2010%5E%7B30%7D%5C%20kg)
So,
![T_1^2=\dfrac{4\pi ^2}{6.67\times 10^{-11}\times 1.989\times 10^{30}}\times 1.496\times 10^{11}\\\\T_1=\sqrt{\dfrac{4\pi^{2}}{6.67\times10^{-11}\times1.989\times10^{30}}\times1.496\times10^{11}}\\\\T_1=2\times 10^{-4}\ s](https://tex.z-dn.net/?f=T_1%5E2%3D%5Cdfrac%7B4%5Cpi%20%5E2%7D%7B6.67%5Ctimes%2010%5E%7B-11%7D%5Ctimes%201.989%5Ctimes%2010%5E%7B30%7D%7D%5Ctimes%201.496%5Ctimes%2010%5E%7B11%7D%5C%5C%5C%5CT_1%3D%5Csqrt%7B%5Cdfrac%7B4%5Cpi%5E%7B2%7D%7D%7B6.67%5Ctimes10%5E%7B-11%7D%5Ctimes1.989%5Ctimes10%5E%7B30%7D%7D%5Ctimes1.496%5Ctimes10%5E%7B11%7D%7D%5C%5C%5C%5CT_1%3D2%5Ctimes%2010%5E%7B-4%7D%5C%20s)
(b) For Sun -Mercury,
![T_2^2=\dfrac{4\pi ^2}{6.67\times 10^{-11}\times 1.989\times 10^{30}}\times 5.79 \times 10^{10}\ m\\\\T_2=\sqrt{\dfrac{4\pi^{2}}{6.67\times10^{-11}\times1.989\times10^{30}}\times 5.79 \times 10^{10}}\ m\\\\T_2=1.31\times 10^{-4}\ s](https://tex.z-dn.net/?f=T_2%5E2%3D%5Cdfrac%7B4%5Cpi%20%5E2%7D%7B6.67%5Ctimes%2010%5E%7B-11%7D%5Ctimes%201.989%5Ctimes%2010%5E%7B30%7D%7D%5Ctimes%205.79%20%5Ctimes%2010%5E%7B10%7D%5C%20m%5C%5C%5C%5CT_2%3D%5Csqrt%7B%5Cdfrac%7B4%5Cpi%5E%7B2%7D%7D%7B6.67%5Ctimes10%5E%7B-11%7D%5Ctimes1.989%5Ctimes10%5E%7B30%7D%7D%5Ctimes%205.79%20%5Ctimes%2010%5E%7B10%7D%7D%5C%20m%5C%5C%5C%5CT_2%3D1.31%5Ctimes%2010%5E%7B-4%7D%5C%20s)
(c) For Sun-Pluto,
![T_3^2=\dfrac{4\pi ^2}{6.67\times 10^{-11}\times 1.989\times 10^{30}}\times 5.91 \times 10^{12}\\\\T_3=\sqrt{\dfrac{4\pi^{2}}{6.67\times10^{-11}\times1.989\times10^{30}}\times 5.91 \times 10^{12}}\\\\T_3=1.32\times 10^{-3}\ s](https://tex.z-dn.net/?f=T_3%5E2%3D%5Cdfrac%7B4%5Cpi%20%5E2%7D%7B6.67%5Ctimes%2010%5E%7B-11%7D%5Ctimes%201.989%5Ctimes%2010%5E%7B30%7D%7D%5Ctimes%205.91%20%5Ctimes%2010%5E%7B12%7D%5C%5C%5C%5CT_3%3D%5Csqrt%7B%5Cdfrac%7B4%5Cpi%5E%7B2%7D%7D%7B6.67%5Ctimes10%5E%7B-11%7D%5Ctimes1.989%5Ctimes10%5E%7B30%7D%7D%5Ctimes%205.91%20%5Ctimes%2010%5E%7B12%7D%7D%5C%5C%5C%5CT_3%3D1.32%5Ctimes%2010%5E%7B-3%7D%5C%20s)
Rock climbing. Free diving. Sky diving. Dog sledding.
<h3>
Answer:</h3>
172.92 °C
<h3>
Explanation:</h3>
Concept being tested: Quantity of heat
We are given;
- Specific heat capacity of copper as 0.09 cal/g°C
- Quantity of heat is 8373 calories
- Mass of copper sample as 538.0 g
We are required to calculate the change in temperature.
- In this case we need to know that the amount of heat absorbed or gained by a substance is given by the product of mass, specific heat capacity and change in temperature.
Therefore, to calculate the change in temperature, ΔT we rearrange the formula;
ΔT = Q ÷ mc
Thus;
ΔT = 8373 cal ÷ (538 g × 0.09 cal/g°C)
= 172.92 °C
Therefore, the change in temperature will be 172.92 °C
when they all are opisite
IDK I just guess