Galaxies are sprawling systems of dust, gas, dark matter, and anywhere from a million to a trillion stars that are held together by gravity. Nearly all large galaxies are thought to also contain supermassive black holes at their centers.
Answer:
![Impulse = 8.0Ns](https://tex.z-dn.net/?f=Impulse%20%3D%20%208.0Ns)
Explanation:
Given
![Force = 80.0N](https://tex.z-dn.net/?f=Force%20%3D%2080.0N)
![Mass = 0.25kg](https://tex.z-dn.net/?f=Mass%20%3D%200.25kg)
![Time = 0.10s](https://tex.z-dn.net/?f=Time%20%3D%200.10s)
Required
Determine the impulse
The impulse is calculated as follows:
![Impulse = Force * Time](https://tex.z-dn.net/?f=Impulse%20%3D%20%20Force%20%2A%20Time)
Substitute values for Force and Time
![Impulse = 80.0N * 0.10s](https://tex.z-dn.net/?f=Impulse%20%3D%20%2080.0N%20%2A%200.10s)
![Impulse = 8.0Ns](https://tex.z-dn.net/?f=Impulse%20%3D%20%208.0Ns)
<em>Hence, the impulse experienced is 8.0Ns</em>
Carbon-14 is naturally created with the interaction of high-energy cosmic rays with atmospheric nitrogen. As part of the atmosphere, living organisms take in the carbon and incorporate this into living tissues. As long as the organism is alive and breathing, it keeps adding new carbon-14. When the organism dies, it stops gaining carbon-14 - or anything else, of course.
Carbon-14 is slightly radioactive, with a half-life of about 5700 years. If we assume that the atmospheric production of carbon-14 has been steady for the last 100,000 years, we can calculate the approximate age of when the organism died by determining what percentage of carbon-14 still exists in the dead material.
Paleo-archaeologists and anthropologists use this information when studying old cultures and civilizations.