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Alecsey [184]
3 years ago
9

A glass tube 1.50 meters long and open at one end is weighted to keep it vertical and is then lowered to the bottom of a lake. W

hen it returns to the surface it is determined that at the bottom of the lake the water rose to within 0.133 meters of the closed end. The lake is 100 meters deep, the air temperature at the surface is 27 "C, atmospheric pressure is 1.01x10s N/m2, and the density of water is 998 kg/m3. a) What is the total pressure at the bottom of the lake

Physics
1 answer:
Lilit [14]3 years ago
3 0

Complete Question

 The complete question is shown on the first uploaded image  

Answer:

The total pressure is  P_T  = 10.79*10^{5} N/m^2

The temperature at the bottom is T_b  = 284.2 \ K

Explanation:

From the question we are told that

    The length of the glass tube is  L  = 1.50 \ m

      The length of water  rise at the bottom of the lake  d = 1.33 \ m

     The depth of the lake is  h =  100 \ m

     The air temperature is T_a   =  27 ^oC =  27 +273 =  300 \ K

      The atmospheric pressure is  P_a = 1.01 *10^{5} N/m

      The density of water is \rho =  998 \ kg/m^3

The total pressure at the bottom of the lake is mathematically represented as

                 P_T  =  P_a + \rho g h

substituting values

               P_T  = 1.01*10^{5}  + 998 * 9.8 * 100

               P_T  = 10.79*10^{5} N/m^2

According to ideal gas law

         At the surface the glass tube not covered by water at surface

             P_a V_a =  nRT_a

Where is the volume of

             P_a *A * L  = nRT_a

 At the bottom of the lake  

           P_T V_b  =  nRT_b

Where V_b is the volume of the glass tube not covered by water at bottom

          and  T_b i the temperature at the bottom

  So the ratio between the temperature  at the surface to the temperature at the bottom is mathematically represented as

             \frac{T_b}{T_a}  =  \frac{d * P_T}{P_a * h}

substituting values

           \frac{T_b}{27}  =  \frac{0.133  * 10.79 *10^5}{1.01 *10^{5} * 1.5}

   =>     T_b  = 284.2 \ K

           

       

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Explanation:

1)

There are three Kepler's law of planetary motion:

  1. 1st law: the planets orbit the sun in elliptical orbits, with the Sun located at one of the 2 focii
  2. 2nd law: a segment connecting the Sun with each planet sweeps out equal areas in equal time intervals. A direct consequence of this is that, when a planet is further from the sun, it travels slower, and when it is closer to the sun, it travels faster
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To solve the problem, we have to write the equation of motions for each block along the direction parallel to the incline.

For the block on the right, we have:

M g sin \theta - T = Ma (1)

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M = 8.0 kg (mass of the block)

g=9.8 m/s^2 (acceleration of gravity)

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For the block on the left, we have similarly

T-mg sin \theta = ma (2)

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m = 3.5 kg (mass of the block)

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From (2) we get

T=mg sin \theta + ma

Substituting into (1),

M g sin \theta - mg sin \theta - ma = Ma

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The tension in the string can be calculated using the equation

T=mg sin \theta + ma

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a=2.2 m/s^2 (acceleration found in part 2)

Substituting,

T=(3.5)(9.8)(sin 35^{\circ}) +(3.5)(2.2)=27.4 N

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Substituting, we find its kinetic energy:

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