Answer:
proteins
Explanation:
protiens is the most difficult nutrient to brek down
To develop this problem it is necessary to apply the concepts given in the balance of forces for the tangential force and the centripetal force. An easy way to detail this problem is through a free body diagram that describes the behavior of the body and the forces to which it is subject.
PART A) Normal Force.
![F_n = \frac{mv^2}{r}](https://tex.z-dn.net/?f=F_n%20%3D%20%5Cfrac%7Bmv%5E2%7D%7Br%7D)
![N+mgcos\theta = \frac{mv^2}{r}](https://tex.z-dn.net/?f=N%2Bmgcos%5Ctheta%20%3D%20%5Cfrac%7Bmv%5E2%7D%7Br%7D)
Here,
Normal reaction of the ring is N and velocity of the ring is v
![N+mgcos\theta = \frac{mv^2}{r}](https://tex.z-dn.net/?f=N%2Bmgcos%5Ctheta%20%3D%20%5Cfrac%7Bmv%5E2%7D%7Br%7D)
![N+Wcos\theta = \frac{W}{g} (\frac{v^2}{r})](https://tex.z-dn.net/?f=N%2BWcos%5Ctheta%20%3D%20%5Cfrac%7BW%7D%7Bg%7D%20%28%5Cfrac%7Bv%5E2%7D%7Br%7D%29)
![N+2cos30\° = \frac{2}{32.2}*\frac{10^2}{2}](https://tex.z-dn.net/?f=N%2B2cos30%5C%C2%B0%20%3D%20%5Cfrac%7B2%7D%7B32.2%7D%2A%5Cfrac%7B10%5E2%7D%7B2%7D)
![N = 1.374lb](https://tex.z-dn.net/?f=N%20%3D%201.374lb)
PART B) Acceleration
![F_t = ma_t](https://tex.z-dn.net/?f=F_t%20%3D%20ma_t)
![-mgsin\theta = ma_t](https://tex.z-dn.net/?f=-mgsin%5Ctheta%20%3D%20ma_t)
![-W sin\theta = \frac{W}{g} a_t](https://tex.z-dn.net/?f=-W%20sin%5Ctheta%20%3D%20%5Cfrac%7BW%7D%7Bg%7D%20a_t)
![-2Sin30\° = (\frac{2}{32.2})a_t](https://tex.z-dn.net/?f=-2Sin30%5C%C2%B0%20%3D%20%28%5Cfrac%7B2%7D%7B32.2%7D%29a_t)
![a_T = -16.10ft/s^2](https://tex.z-dn.net/?f=a_T%20%3D%20-16.10ft%2Fs%5E2)
Negative symbol indicates deceleration.
<em>NOTE: For the problem, the graph in which the turning radius and the angle of suspension was specified was not supplied. A graphic that matches the description given by the problem is attached.</em>
A solar eclipse will be visible over a wide area of the north polar region
on Friday, March 20.
England is not in the path of totality, but it's close enough so that a large
part of the sun will be covered, and it will be a spectacular sight.
For Londoners, the eclipse begins Friday morning at 8:25 AM,when the
moon just begins to eat away at the sun's edge. It advances slowly, as more
and more of the sun disappears, and reaches maximum at 9:31 AM. Then
the obscured part of the sun begins to shrink, and the complete disk is
restored by the end of the eclipse at 10:41AM, after a period of 2 hours
16 minutes during which part of the sun appears to be missing.
The catch in observing the eclipse is:
<em><u>YOU MUST NOT LOOK AT THE SUN</u></em>.
Staring at the sun for a period of time can cause permanent damage to
your vision, even though <em><u>you don't feel it while it's happening</u></em>.
This is not a useful place to try and give you complete instructions or
suggestions for observing the sun over a period of hours. Please look
in your local newspaper, or search online for phrases like "safe eclipse
viewing".