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Solving for a Variable Solve the equation for the indicated variable. $$P V=n R T ; \quad \text { for } R$$

Short Answer

Expert verified
The solution is \( R = \frac{PV}{nT} \).

Step by step solution

01

Understand the Given Equation

The given equation is \( PV = nRT \). This equation is the ideal gas law, and we need to solve it for \( R \). It relates pressure \( P \), volume \( V \), number of moles \( n \), ideal gas constant \( R \), and temperature \( T \).
02

Isolating Variable R

To solve for \( R \), we need to isolate it on one side of the equation. We can do this by dividing both sides of the equation by \( nT \). This gives us the equation \( R = \frac{PV}{nT} \).
03

Verify the Solution

Check the solution by considering the units. The units for \( R \) should agree with those of \( P \), \( V \), \( n \), and \( T \): pressure times volume divided by moles and temperature \( (pressure \cdot volume)/(moles \cdot temperature) \). This confirms that \( R = \frac{PV}{nT} \) is dimensionally correct.

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Key Concepts

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

Equation Solving
Whenever we look at an equation, we are seeing a balance between two sides. The initial goal in equation solving is to identify what is given and what is needed. In the Ideal Gas Law equation, which is \( PV = nRT \), our task is to find \( R \), the ideal gas constant. This means we'll adjust the equation to express \( R \) in terms of the other variables. To solve an equation:
  • Understand the purpose and arrangement - here, the Ideal Gas Law shows the relation between several properties of a gas.
  • Identify the target variable. In this case, \( R \) is our target.
  • Use algebraic operations to rearrange the equation.
In simple terms, solve the equation one step at a time, like unraveling a yarn until you get to the desired variable.
Isolating Variables
To solve equations effectively, you must know how to isolate variables. Isolating a variable means getting it alone on one side of the equation, free from any other numbers or letters. In the example equation \( PV = nRT \), isolating \( R \) requires us to remove \( n \) and \( T \) from its right-hand side.Here's a simple way to think about it:- Division and multiplication are useful tools. They help break down the equation.To isolate \( R \), divide both sides by \( nT \). This operation gives us\(R = \frac{PV}{nT}\)
  • Division cancels multiplication. Since \( n \) and \( T \) multiply \( R \), dividing by them cancels them out.
  • Remember, whatever you do to one side of the equation, do it to the other.
Dimensional Analysis
Dimensional analysis is a way to check if your equations make sense. It involves looking at units (like meters, liters, or pascals) to make sure your equation is balanced. After isolating \( R \) in the equation \( R = \frac{PV}{nT} \), checking the dimensions ensures that everything is correct.Here's how to do it:- Identify the units of each variable in the equation: - Pressure \( P \) is in pascals - Volume \( V \) is in liters - Moles \( n \) have no units - Temperature \( T \) is in KelvinCompare with \( R \)'s expected units:
  • Pressure \( \times \) Volume results in L.Pa
  • Moles \( \times \) Temperature leads to mol.K
Balancing the equation, we find that \( R \) has units of L.Pa/mol.K, verifying that our solution \( R = \frac{PV}{nT} \) is dimensionally consistent. This kind of check is crucial because it confirms you've considered all the physical aspects correctly.

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Most popular questions from this chapter

Complete the squares in the general equation \(x^{2}+a x+y^{2}+b y+c=0\) and simplify the result as much as possible. Under what conditions on the coefficients \(a, b,\) and \(c\) does this equation represent a circle? A single point? The empty set? In the case in which the equation does represent a circle, find its center and radius.

It follows from Kepler's Third Law of planetary motion that the average distance from a planet to the sun (in meters) is $$d=\left(\frac{G M}{4 \pi^{2}}\right)^{1 / 3} T^{2 / 3}$$ where \(M=1.99 \times 10^{30} \mathrm{kg}\) is the mass of the sun, \(G=6.67 \times 10^{-11} \mathrm{N} \cdot \mathrm{m}^{2} / \mathrm{kg}^{2}\) is the gravitational constant, and \(T\) is the period of the planet's orbit (in seconds). Use the fact that the period of the earth's orbit is about 365.25 days to find the distance from the earth to the sun.

Write the number indicated in each statement in scientific notation. (a) A light-year, the distance that light travels in one year, is about \(5,900,000,000,000 \mathrm{mi}\) (b) The diameter of an electron is about \(0.0000000000004 \mathrm{cm}\) (c) A drop of water contains more than 33 billion billion molecules.

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Use scientific notation, the Laws of Exponents, and a calculator to perform the indicated operations. State your answer rounded to the number of significant digits indicated by the given data. $$\frac{(73.1)\left(1.6341 \times 10^{28}\right)}{0.0000000019}$$

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