<span><u><em>A</em></u><em><u></u></em><em><u></u></em><u><em> long-lived, high-pressure storm on jupiter a place where reddish particles from io impact jupiter's surface</em></u></span><u><em> </em></u>
Answer:
The more possible energy you can exert, the higher the potential energy
Explanation:
Answer:
0.152724283058 rad/s
Explanation:
In this system the angular momentum is conserved
Change in angular velocity is
The change in angular velocity is 0.152724283058 rad/s
<h3>SOLUTION:</h3>
<u>=</u><u>)</u><u> </u><u>acceleration</u><u>:</u>
<u>=</u><u>)</u><u>velocity</u><u>/</u><u>time</u>
<u>=</u><u>)</u><u> </u><u>4</u><u>0</u><u>0</u><u>/</u><u>1</u><u>2</u><u>0</u>
<u>=</u><u>)</u><u> </u><u>1</u><u>0</u><u>/</u><u>3</u><u> </u><u>or</u><u> </u><u>3</u><u>.</u><u>3</u><u>3</u>
Answer:
There is a dependency relationship between the refractive index of each substance and the radiation wavelength.
The refractive index in a given medium is inversely proportional to the wavelength of a color.
For example:
The rays of the red color have a wavelength greater than the rays of the blue color, therefore they have a lower refractive index and consequently a light scattering less than the blue.
Snell's law :
n₂/n₁ = v₁/v₂ = λ₁ /λ₂
*n: (refractive index)
v: (speed of light propagation)
λ: (wavelength)