Answer:
<u>EFFECTS: ( doughts)</u>
- There would be less water in the river for you and other people who live along the river to use.
- If we use too much water during times of normal rainfall, we might not have enough water when a drought happens.
<u>EFFECTS:( FLOODS)</u>
- The immediate impacts of flooding include loss of human life, damage to property, destruction of crops, loss of livestock, and deterioration of health conditions owing to waterborne diseases.
- power plants, roads and bridges are damaged and disrupted, some economic activities may come to a standstill, people are forced to leave their homes and normal life is disrupted.
How to prevent from flooding is :
- Construct buildings above flood levels.
- Tackle climate change
How to prevent from droughts :
- drought trends that may occur based on statistical and actual weather forecasts.
- In the U.S., the U.S. Drought Monitor provides a day-by-day visual of the drought conditions around the country.
* Hopefully this helps:) Mark me the brainliest:)!!!
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Answer:
electromagnetic wave i think
Explanation:
Answer:
A) True
Explanation:
Researchers have detected numerous jets of gas ejected from poles of young stars and planetary nebulae.
By examining images of hydrogen molecules excited at infrared wavelengths, scientists have been able to see through the gas and dust in the Milky Way, in order to observe the most distant targets. These goals are normally hidden from view and many of them have never been seen before.
The entire study area covers approximately 1,450 times the size of the full moon, or the equivalent of an image of 95 gigapixels. The survey reveals jets emanating from proto-stars and planetary nebulas, as well as remnants of supernovae, the illuminated edges of vast clouds of gas and dust, and the warm regions that surround massive stars and their associated groups of smaller stars.
Answer:
The answer is "
".
Explanation:
Formula for calculating the mass in He:
![\to m = \frac{PV}{RT}\\](https://tex.z-dn.net/?f=%5Cto%20m%20%3D%20%5Cfrac%7BPV%7D%7BRT%7D%5C%5C)
![= \frac{500 \times 1}{ 2.0769 \times (40 + 273)}\\\\ = \frac{500 }{ 2.0769 \times 313}\\\\ = \frac{500 }{ 650.0697}\\\\= 0.76914 \ Kg](https://tex.z-dn.net/?f=%3D%20%5Cfrac%7B500%20%5Ctimes%201%7D%7B%202.0769%20%5Ctimes%20%2840%20%2B%20273%29%7D%5C%5C%5C%5C%20%3D%20%5Cfrac%7B500%20%7D%7B%202.0769%20%5Ctimes%20313%7D%5C%5C%5C%5C%20%3D%20%5Cfrac%7B500%20%7D%7B%20650.0697%7D%5C%5C%5C%5C%3D%200.76914%20%5C%20Kg)
Formula for calculating the mass in
:
![\to m = \frac{PV}{RT}\\](https://tex.z-dn.net/?f=%5Cto%20m%20%3D%20%5Cfrac%7BPV%7D%7BRT%7D%5C%5C)
![= \frac{500 \times 1}{ 0.2968 \times (120+ 273)}\\\\ = \frac{500 }{ 0.2968 \times 393}\\\\ = \frac{500 }{ 116.6424}\\\\= 4.2866\ Kg](https://tex.z-dn.net/?f=%3D%20%5Cfrac%7B500%20%5Ctimes%201%7D%7B%200.2968%20%5Ctimes%20%28120%2B%20273%29%7D%5C%5C%5C%5C%20%3D%20%5Cfrac%7B500%20%7D%7B%200.2968%20%5Ctimes%20393%7D%5C%5C%5C%5C%20%3D%20%5Cfrac%7B500%20%7D%7B%20116.6424%7D%5C%5C%5C%5C%3D%204.2866%5C%20Kg)
by using the temperature balancing the equation:
![T' = \frac{mcT (He) + mcT ( N_2 )}{ mc (He) + mc ( N_2)}](https://tex.z-dn.net/?f=T%27%20%3D%20%5Cfrac%7BmcT%20%28He%29%20%2B%20mcT%20%28%20N_2%20%29%7D%7B%20mc%20%28He%29%20%2B%20mc%20%28%20N_2%29%7D)
![= \frac{0.76914 \times 3.1156 \times 313 + 4.2866 \times 0.743 \times393}{ 0.76914 \times 3.1156 + 4.2866 \times 0.743} \\\\ = 357 \ \ K \approx 83.8^{\circ} \ C](https://tex.z-dn.net/?f=%3D%20%5Cfrac%7B0.76914%20%5Ctimes%203.1156%20%5Ctimes%20313%20%2B%204.2866%20%5Ctimes%200.743%20%5Ctimes393%7D%7B%20%200.76914%20%5Ctimes%203.1156%20%2B%204.2866%20%5Ctimes%200.743%7D%20%5C%5C%5C%5C%20%3D%20357%20%20%5C%20%5C%20K%20%5Capprox%20%2083.8%5E%7B%5Ccirc%7D%20%5C%20C)