/*! This file is auto-generated */ .wp-block-button__link{color:#fff;background-color:#32373c;border-radius:9999px;box-shadow:none;text-decoration:none;padding:calc(.667em + 2px) calc(1.333em + 2px);font-size:1.125em}.wp-block-file__button{background:#32373c;color:#fff;text-decoration:none} Problem 61 A large tank of water has a hose... [FREE SOLUTION] | 91影视

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A large tank of water has a hose connected to it (Fig. P18.61). The tank is sealed at the top and has compressed air between the water surface and the top. When the water height \(h\) has the value \(3.50 \mathrm{~m}\), the absolute pressure \(p\) of the compressed air is \(4.20 \times 10^{5} \mathrm{~Pa}\). Assume that the air above the water expands at constant temperature, and take the atmospheric pressure to be \(1.00 \times 10^{5} \mathrm{~Pa}\). (a) What is the speed with which water flows out of the hose when \(h=3.50 \mathrm{~m} ?\) (b) As water flows out of the tank, \(h\) decreases. Calculate the speed of flow for \(h=3.00 \mathrm{~m}\) and for \(h=2.00 \mathrm{~m} .\) (c) At what value of \(h\) does the flow stop?

Short Answer

Expert verified
The speed with which water flows out of the hose when \(h=3.50 m\) is approximately \(8.14 m/s\). When \(h = 3.00 m\) the speed is approximately \(7.27 m/s\) and when \(h=2.00 m\), the speed is approximately \(5.42 m/s\). The outflow of water will stop when \(h\) is approximately \(1.07 m\).

Step by step solution

01

Bernoulli's Principle

First, using Bernoulli's equation which is \(P + \frac{1}{2}蟻v^2 + 蟻gh = const\), where \(P\) is the pressure, \(v\) is the velocity, \(蟻\) is the density of the fluid, and \(h\) is the height. In this case, apply this to both inside the tank and at the exit of the hose. Inside the tank water is at rest, so \(v = 0\). This gives us : \(P_{air} + 蟻_{water}gh = P_{atm} + \frac{1}{2}蟻_{water}v^2\).
02

Solve for water velocity when h=3.5m

Plug in given values and isolate \(v\). \(P_{air} = 4.20 \times 10^{5} Pa\), \(P_{atm} = 1.00 \times 10^{5} Pa\), \(蟻_{water} = 1000 kg/m^3\), and \(g = 9.8 m/s^2\). Solving for \(v\) when \(h = 3.50 m\) gives \(v = \sqrt{\frac{2(P_{air} + 蟻_{water}gh - P_{atm})}{蟻_{water}}}\). Calculate the values.
03

Solve for water velocity when h=3.0m and h=2.0m

Apply the same formula as step 2 with values of \(h = 3.00 m\) and \(h = 2.00 m\).
04

Determine when the water flow stops

The water will stop flowing when the pressure of the air equals the atmospheric pressure because then the forces will balance out. Therefore, \(h\) when \(P_{air} = P_{atm}\). Use the ideal gas law \(PV = nRT\) assuming \(nRT = const\) (temperature and amount of air mass is constant), so \(P_1V_1 = P_2V_2\). Substituting \(V = Ah\) (A is the cross-sectional area of the tank and h is height), we get \(P_{1}h_{1} = P_{2}h_{2}\) also since \(P_2 = P_{atm}\), solve for \(h_2\).

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Key Concepts

These are the key concepts you need to understand to accurately answer the question.

Fluid Dynamics
Fluid dynamics is the study of how fluids (liquids and gases) move. In our exercise, water flows from a tank through a hose, which is a good example of fluid dynamics at work. The key to understanding this concept is realizing that fluid flow can change under different conditions. There are several factors that affect fluid movement, such as:
  • Viscosity: This measures how thick or sticky a fluid is. Water has low viscosity, which allows it to flow easily.
  • Flow rate: This is the volume of fluid that moves through a section of the system per unit of time.
  • Flow type: Fluids can have laminar (smooth and orderly) or turbulent (rough and chaotic) flow. In this case, since the air in the tank is compressed and the water flows out, it鈥檚 more likely to be turbulent if the flow speed increases.
  • Bernoulli鈥檚 principle: An important part of fluid dynamics, it tells us how fluid pressure, fluid velocity, and height are related.
By understanding these factors, it becomes easier to analyze and predict how the water behaves as it exits the hose.
Pressure
Pressure is a measure of how much force is applied over a certain area. In our problem, pressure plays a crucial role in determining how fast the water exits the hose. The compressed air in the tank creates pressure on the water surface. This pressure is higher than atmospheric pressure, thus forcing water out through the hose.
The critical points about pressure in fluid dynamics include:
  • Absolute pressure: This is the total pressure experienced at any point. In our tank, the absolute pressure includes both the atmospheric pressure and the pressure from the compressed air.
  • Gauge pressure: This measures the pressure relative to atmospheric pressure. In many problems, knowing this is enough because atmospheric pressure is constant at sea level.
  • Pressure gradient: Differences in pressure between two points can set fluids in motion. In the tank, pressure differences push the water through the hose.
Understanding the relationships among these pressure concepts, and how they interact with fluid dynamics, is crucial for solving problems like this one.
Velocity of Fluid Flow
The velocity of fluid flow refers to the speed at which the fluid moves through a section of the system. This velocity is governed by several factors:
  • Bernoulli鈥檚 equation: This equation relates the velocity of a fluid to pressure and height, showing that a decrease in pressure or an increase in height accompanies an increase in the fluid's velocity.
  • Continuity equation: This states that the flow rate must remain constant in a closed system. Thus, if a fluid enters a narrower section of a pipe, it has to speed up to maintain flow rate.
In the problem鈥檚 context, when Bernoulli鈥檚 equation is applied at two points (inside the tank and at the hose outlet), it allows us to calculate the exit velocity of water by understanding how the pressures and heights at these points differ.
For example, as water leaves the tank, the height decreases, affecting the velocity according to the equation. As the height further decreases to points like 3.0 and 2.0 meters, the velocity will change accordingly. This interplay is critical in determining how fast water flows out through the hose.
Ideal Gas Law
The ideal gas law is an important relation in physics that connects pressure, volume, and temperature of a gas. Its formula is expressed as:
\( PV = nRT \)
Where:
  • \( P \) is the pressure.
  • \( V \) is the volume.
  • \( n \) is the number of moles of gas.
  • \( R \) is the gas constant.
  • \( T \) is the temperature.
This law assumes that the gas behaves ideally, meaning there are no intermolecular forces and the gas molecules occupy negligible space. In this problem:
  • The air above the water is treated as an ideal gas with a constant temperature as the water flows out.
  • The compressed air鈥檚 pressure affects how it expands as the water leaves, showing that pressure and volume have an inverse relationship when temperature is constant (Boyle鈥檚 Law).
In the exercise, we use this law to determine when the water flow will stop. This happens when the compressed air pressure drops to equal the atmospheric pressure, allowing us to find the specific water height where this occurs.

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Most popular questions from this chapter

A physics lecture room at 1.00 atm and \(27.0^{\circ} \mathrm{C}\) has a volume of \(216 \mathrm{~m}^{3}\). (a) Use the ideal-gas law to estimate the number of air molecules in the room. Assume that all of the air is \(\mathrm{N}_{2} .\) Calculate (b) the particle density - that is, the number of \(\mathrm{N}_{2}\), molecules per cubic centimeter-and (c) the mass of the air in the room.

The vapor pressure is the pressure of the vapor phase of a substance when it is in equilibrium with the solid or liquid phase of the substance. The relative humidity is the partial pressure of water vapor in the air divided by the vapor pressure of water at that same temperature, expressed as a percentage. The air is saturated when the humidity is \(100 \%\). (a) The vapor pressure of water at \(20.0^{\circ} \mathrm{C}\) is \(2.34 \times 10^{3} \mathrm{~Pa}\). If the air temperature is \(20.0^{\circ} \mathrm{C}\) and the relative humidity is \(60 \%,\) what is the partial pressure of water vapor in the atmosphere (that is, the pressure due to water vapor alone)? (b) Under the conditions of part (a), what is the mass of water in \(1.00 \mathrm{~m}^{3}\) of air? (The molar mass of water is \(18.0 \mathrm{~g} / \mathrm{mol}\). Assume that water vapor can be treated as an ideal gas.)

A balloon of volume \(750 \mathrm{~m}^{3}\) is to be filled with hydrogen at atmospheric pressure \(\left(1.01 \times 10^{5} \mathrm{~Pa}\right) .\) (a) If the hydrogen is stored in cylinders with volumes of \(1.90 \mathrm{~m}^{3}\) at a gauge pressure of \(1.20 \times 10^{6} \mathrm{~Pa}\), how many cylinders are required? Assume that the temperature of the hydrogen remains constant. (b) What is the total weight (in addition to the weight of the gas) that can be supported by the balloon if both the gas in the balloon and the surrounding air are at \(15.0^{\circ} \mathrm{C} ?\) The molar mass of hydrogen \(\left(\mathrm{H}_{2}\right)\) is \(2.02 \mathrm{~g} / \mathrm{mol} .\) The density of air at \(15.0^{\circ} \mathrm{C}\) and atmospheric pressure is \(1.23 \mathrm{~kg} / \mathrm{m}^{3} .\) See Chapter 12 for a discussion of buoyancy. (c) What weight could be supported if the balloon were filled with helium (molar mass \(4.00 \mathrm{~g} / \mathrm{mol}\) ) instead of hydrogen, again at \(15.0^{\circ} \mathrm{C} ?\)

The dark area in Fig. \(\mathbf{P} 18.83\) that appears devoid of stars is a dark nebula, a cold gas cloud in interstellar space that contains enough material to block out light from the stars behind it. A typical dark nebula is about 20 light-years in diameter and contains about 50 hydrogen atoms per cubic centimeter (monatomic hydrogen, not \(\mathrm{H}_{2}\) ) at about \(20 \mathrm{~K}\). (A lightyear is the distance light travels in vacuum in one year and is equal to \(\left.9.46 \times 10^{15} \mathrm{~m} .\right)\) (a) Estimate the mean free path for a hydrogen atom in a dark nebula. The radius of a hydrogen atom is \(5.0 \times 10^{-11} \mathrm{~m}\). (b) Estimate the rms speed of a hydrogen atom and the mean free time (the average time between collisions for a given atom). Based on this result, do you think that atomic collisions, such as those leading to \(\mathrm{H}_{2} \mathrm{~mol}-\) ecule formation, are very important in determining the composition of the nebula? (c) Estimate the pressure inside a dark nebula. (d) Compare the rms speed of a hydrogen atom to the escape speed at the surface of the nebula (assumed spherical). If the space around the nebula were a vacuum, would such a cloud be stable or would it tend to evaporate? (e) The stability of dark nebulae is explained by the presence of the interstellar medium (ISM), an even thinner gas that permeates space and in which the dark nebulae are embedded. Show that for dark nebulae to be in equilibrium with the ISM, the numbers of atoms per volume \((N / V)\) and the temperatures \((T)\) of dark nebulae and the ISM must be related by $$ \frac{(N / V)_{\text {nebula }}}{(N / V)_{\text {ISM }}}=\frac{T_{\text {ISM }}}{T_{\text {nebula }}} $$ (f) In the vicinity of the sun, the ISM contains about 1 hydrogen atom per \(200 \mathrm{~cm}^{3} .\) Estimate the temperature of the ISM in the vicinity of the sun. Compare to the temperature of the sun's surface, about \(5800 \mathrm{~K}\). Would a spacecraft coasting through interstellar space burn up? Why or why not?

(a) Calculate the mass of nitrogen present in a volume of \(3000 \mathrm{~cm}^{3}\) if the gas is at \(22.0^{\circ} \mathrm{C}\) and the absolute pressure of \(2.00 \times 10^{-13}\) atm is a partial vacuum easily obtained in laboratories. (b) What is the density (in \(\mathrm{kg} / \mathrm{m}^{3}\) ) of the \(\mathrm{N}_{2}\) ?

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