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masya89 [10]
1 year ago
10

In order for the ball to be able to make a complete circle around the peg, there must be sufficient speed at the top of its arc

such that the centripetal acceleration is large enough to keep the string that. Determine the minimum speed for the ball to achieve a complete circle in terms of L, d, and g. (Hint: use Newton’s 2nd Law and consider what the string tension must be for the ball to just barely get over the top).
Physics
1 answer:
Vesna [10]1 year ago
6 0

Answer:

Explanation:

Let T be the tension in the swing

At top point mg-T=\frac{mv^2}{r}

where v=velocity needed to complete circular path

r=distance between point of  rotation to the ball center=L+\frac{d}{2} (d=diameter of ball)

Th-resold velocity is given by mg-0=\frac{mv^2}{r}

To get the velocity at bottom conserve energy at Top and bottom

At top E_T=mg\times 2L+\frac{mv^2}{2}

Energy at Bottom E_b=\frac{mv_0^2}{2}

Comparing two as energy is conserved

v_0^2=4gr+gr

v_0^2=5gr

v_0=\sqrt{5gr}

v_0=\sqrt{5g\left ( \frac{d}{2}+L\right )}

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Answer:

Explanation:

Using the efficiency formula;

Efficiency = Work done by the machine (output)/work done on the machine (input) ×100%

Efficiency =w/50 ×100

90 = 100w/50

Cross multiply

90×50 = 100W

4500 = 100W

W = 4500/100

W = 45Joules

Hence the lever does 45Joules of work on its load

2) Mechanical Advantage= Load/Effort

Given

MA = 4

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Effort = 500/4

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1 year ago
A couch is pushed with a horizontal force of 80 N and moves the couch a
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400 J

Explanation:

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Consider a star that is a sphere with a radius of 6.32 108 m and an average surface temperature of 5350 K. Determine the amount
Mariulka [41]

Answer:

The value is  \Delta s  = 8.537 *10^{25 } \ J/K

Explanation:

From the we are told that

   The radius of the sphere is r =  6.32 *10^{8} \  m

   The temperature is T_x  =  5350 \  K

    The average temperature of the rest of the universe is  T_r  =  2.73 \  K

Generally the change in entropy of the entire universe per second is mathematically represented as

         \Delta s  =  s_r - s_x

Here s_r is the entropy of the rest of the universe which is mathematically represented as

          s_r =  \frac{Q}{T_r}

Here Q is the quantity of heat radiated by the star which is mathematically represented as

           Q =  4 \pi *  r^2 *  \sigma * T^4_x

Here \sigma is the Stefan-Boltzmann constant with value  

           \sigma =  5.67 * 10^{-8 }W\cdot  m^{-2} \cdot  K^{-4}.

=>         Q =  4 \pi *  (6.32*10^{8})^2 *  5.67 * 10^{-8 }  * 5350 ^4

=>         Q =  2.332 *10^{26} \  J

So

      s_r =  \frac{2.332 *10^{26}}{2.73}

=>   s_r =  8.5415 *10^{25}\  J/K

Here s_x is the entropy of the rest of the universe which is mathematically represented as

      s_x =  \frac{Q}{T_x}

=>   s_x =  \frac{2.332 *10^{26} }{5350}

=>   s_x =  4.359 *10^{22} \  J/K

So

      \Delta s  = 8.5415 *10^{25}  - 4.359 *10^{22}

=>   \Delta s  = 8.537 *10^{25 } \ J/K

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The difference in heights of the liquid in the two sides of the manometer is 43.4 cm when the atmospheric pressure is 755 mm hg.
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The atmospheric P is greater than the P in the flask, since the Hg level is lacking down lower on the side open to the atmosphere. 

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435 mm manometer liquid x (1 mm Hg / 17.2 mm manometer liquid) = 25.3 mm Hg 

The pressure in the flask is 755 - 25.3 = 729.7 mmHg. 

729.7 mmHg x (1 atm / 760 mmHg ) = 0.960 atm.

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