If an ideal gas has a pressure of 6.590 x 10° Pa, a temperature of 43.00 °C, and a volume of 0.0127 m², how many moles n of gas are in the sample? n = mol
If an ideal gas has a pressure of 6.590 x 10° Pa, a temperature of 43.00 °C, and a volume of 0.0127 m², how many moles n of gas are in the sample? n = mol
College Physics
11th Edition
ISBN:9781305952300
Author:Raymond A. Serway, Chris Vuille
Publisher:Raymond A. Serway, Chris Vuille
Chapter1: Units, Trigonometry. And Vectors
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![**Ideal Gas Law Calculation**
If an ideal gas has a pressure of \(6.590 \times 10^5 \, \text{Pa}\), a temperature of \(43.00 \, ^\circ \text{C}\), and a volume of \(0.0127 \, \text{m}^3\), how many moles \(n\) of gas are in the sample?
\(n =\) [Answer box]
**Explanation:**
To find the number of moles \(n\) of the gas, use the ideal gas law equation \(PV = nRT\), where:
- \(P\) is the pressure,
- \(V\) is the volume,
- \(n\) is the number of moles,
- \(R\) is the ideal gas constant (\(8.314 \, \text{J/mol·K}\)),
- \(T\) is the temperature in Kelvin.
Convert temperature from Celsius to Kelvin by adding 273.15. Calculate \(n\) using the rearranged equation \(n = \frac{PV}{RT}\).](/v2/_next/image?url=https%3A%2F%2Fcontent.bartleby.com%2Fqna-images%2Fquestion%2F91f424ac-8f96-4172-b739-006cab2e5691%2F050765cf-07e2-4440-b19d-ca423c7d6664%2F9aghvl_processed.jpeg&w=3840&q=75)
Transcribed Image Text:**Ideal Gas Law Calculation**
If an ideal gas has a pressure of \(6.590 \times 10^5 \, \text{Pa}\), a temperature of \(43.00 \, ^\circ \text{C}\), and a volume of \(0.0127 \, \text{m}^3\), how many moles \(n\) of gas are in the sample?
\(n =\) [Answer box]
**Explanation:**
To find the number of moles \(n\) of the gas, use the ideal gas law equation \(PV = nRT\), where:
- \(P\) is the pressure,
- \(V\) is the volume,
- \(n\) is the number of moles,
- \(R\) is the ideal gas constant (\(8.314 \, \text{J/mol·K}\)),
- \(T\) is the temperature in Kelvin.
Convert temperature from Celsius to Kelvin by adding 273.15. Calculate \(n\) using the rearranged equation \(n = \frac{PV}{RT}\).
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