Sorry don’t know this one
Answer:
<em>Infrared telescope and camera</em>
<em></em>
Explanation:
An infrared telescope uses infrared light to detect celestial bodies. The infrared radiation is one of the known forms of electromagnetic radiation. Infrared radiation is given off by a body possessing some form of heat. All bodies above the absolute zero temperature in the universe radiates some form of heat, which can then be detected by an infrared telescope, and infrared radiation can be used to study or look into a system that is void of detectable visible light.
Stars are celestial bodies that are constantly radiating heat. In order to see a clearer picture of the these bodies, <em>Infrared images is better used, since they are able to penetrate the surrounding clouds of dust,</em> and have located many more stellar components than any other types of telescope, especially in dusty regions of star clusters like the Trapezium cluster.
I believe it she should use the first aid kit next
Answer:
![P = 1.090\,N](https://tex.z-dn.net/?f=P%20%3D%201.090%5C%2CN)
Explanation:
The constant speed means that ball is not experimenting acceleration. This elements is modelled by using the following equation of equilibrium:
![\Sigma F = P - W + F_{D}](https://tex.z-dn.net/?f=%5CSigma%20F%20%3D%20P%20-%20W%20%2B%20F_%7BD%7D)
![\Sigma F = P - \rho \cdot V \cdot g + c\cdot v = 0](https://tex.z-dn.net/?f=%5CSigma%20F%20%3D%20P%20-%20%5Crho%20%5Ccdot%20V%20%5Ccdot%20g%20%2B%20c%5Ccdot%20v%20%3D%200)
Now, the exerted force is:
![P = \rho \cdot V \cdot g - c\cdot v](https://tex.z-dn.net/?f=P%20%3D%20%5Crho%20%5Ccdot%20V%20%5Ccdot%20g%20-%20c%5Ccdot%20v)
The volume of a sphere is:
![V = \frac{4\cdot \pi}{3}\cdot R^{3}](https://tex.z-dn.net/?f=V%20%3D%20%5Cfrac%7B4%5Ccdot%20%5Cpi%7D%7B3%7D%5Ccdot%20R%5E%7B3%7D)
![V = \frac{4\cdot \pi}{3}\cdot (0.014\,m)^{3}](https://tex.z-dn.net/?f=V%20%3D%20%5Cfrac%7B4%5Ccdot%20%5Cpi%7D%7B3%7D%5Ccdot%20%280.014%5C%2Cm%29%5E%7B3%7D)
![V = 1.149\times 10^{-5}\,m^{3}](https://tex.z-dn.net/?f=V%20%3D%201.149%5Ctimes%2010%5E%7B-5%7D%5C%2Cm%5E%7B3%7D)
Lastly, the force is calculated:
![P = (8910\,\frac{kg}{m^{3}} )\cdot (1.149\cdot 10^{-5}\,m^{3})\cdot (9.81\,\frac{m}{s^{2}} )+(0.950\,\frac{kg}{s})\cdot (0.09\,\frac{m}{s} )](https://tex.z-dn.net/?f=P%20%3D%20%288910%5C%2C%5Cfrac%7Bkg%7D%7Bm%5E%7B3%7D%7D%20%29%5Ccdot%20%281.149%5Ccdot%2010%5E%7B-5%7D%5C%2Cm%5E%7B3%7D%29%5Ccdot%20%289.81%5C%2C%5Cfrac%7Bm%7D%7Bs%5E%7B2%7D%7D%20%29%2B%280.950%5C%2C%5Cfrac%7Bkg%7D%7Bs%7D%29%5Ccdot%20%280.09%5C%2C%5Cfrac%7Bm%7D%7Bs%7D%20%29)
![P = 1.090\,N](https://tex.z-dn.net/?f=P%20%3D%201.090%5C%2CN)
Velocity is the rate of change of position with respect to time, whereas acceleration is the rate of change of velocity. Both are vector quantities (and so also have a specified direction), but the units of velocity are meters per second while the units of acceleration are meters per second squared.