Standard temperature and pressure (STP) is a crucial concept in gas calculations, providing a reference point for various scientific measurements. At STP, the temperature is defined as 0 degrees Celsius, which is equivalent to 273.15 Kelvin. It is important to use Kelvin for gas calculations, as it is the absolute temperature scale. Additionally, the pressure at STP is set at 1 atmosphere (atm). Therefore, when referring to STP, remember that it signifies a temperature of 273.15 K and a pressure of 1 atm, which are essential for accurately applying gas laws and performing calculations in chemistry.
- 1. Matter and Measurements4h 31m
- What is Chemistry?7m
- The Scientific Method9m
- Classification of Matter16m
- States of Matter8m
- Physical & Chemical Changes19m
- Chemical Properties8m
- Physical Properties5m
- Intensive vs. Extensive Properties13m
- Temperature (Simplified)9m
- Scientific Notation13m
- SI Units (Simplified)5m
- Metric Prefixes24m
- Significant Figures (Simplified)11m
- Significant Figures: Precision in Measurements7m
- Significant Figures: In Calculations19m
- Conversion Factors (Simplified)15m
- Dimensional Analysis22m
- Density12m
- Specific Gravity9m
- Density of Geometric Objects19m
- Density of Non-Geometric Objects9m
- 2. Atoms and the Periodic Table5h 23m
- The Atom (Simplified)9m
- Subatomic Particles (Simplified)12m
- Isotopes17m
- Ions (Simplified)22m
- Atomic Mass (Simplified)17m
- Atomic Mass (Conceptual)12m
- Periodic Table: Element Symbols6m
- Periodic Table: Classifications11m
- Periodic Table: Group Names8m
- Periodic Table: Representative Elements & Transition Metals7m
- Periodic Table: Elemental Forms (Simplified)6m
- Periodic Table: Phases (Simplified)8m
- Law of Definite Proportions9m
- Atomic Theory9m
- Rutherford Gold Foil Experiment9m
- Wavelength and Frequency (Simplified)5m
- Electromagnetic Spectrum (Simplified)11m
- Bohr Model (Simplified)9m
- Emission Spectrum (Simplified)3m
- Electronic Structure4m
- Electronic Structure: Shells5m
- Electronic Structure: Subshells4m
- Electronic Structure: Orbitals11m
- Electronic Structure: Electron Spin3m
- Electronic Structure: Number of Electrons4m
- The Electron Configuration (Simplified)22m
- Electron Arrangements5m
- The Electron Configuration: Condensed4m
- The Electron Configuration: Exceptions (Simplified)12m
- Ions and the Octet Rule9m
- Ions and the Octet Rule (Simplified)8m
- Valence Electrons of Elements (Simplified)5m
- Lewis Dot Symbols (Simplified)7m
- Periodic Trend: Metallic Character4m
- Periodic Trend: Atomic Radius (Simplified)7m
- 3. Ionic Compounds2h 18m
- Periodic Table: Main Group Element Charges12m
- Periodic Table: Transition Metal Charges6m
- Periodic Trend: Ionic Radius (Simplified)5m
- Periodic Trend: Ranking Ionic Radii8m
- Periodic Trend: Ionization Energy (Simplified)9m
- Periodic Trend: Electron Affinity (Simplified)8m
- Ionic Bonding6m
- Naming Monoatomic Cations6m
- Naming Monoatomic Anions5m
- Polyatomic Ions25m
- Naming Ionic Compounds11m
- Writing Formula Units of Ionic Compounds7m
- Naming Ionic Hydrates6m
- Naming Acids18m
- 4. Molecular Compounds2h 18m
- Covalent Bonds6m
- Naming Binary Molecular Compounds6m
- Molecular Models4m
- Bonding Preferences6m
- Lewis Dot Structures: Neutral Compounds (Simplified)8m
- Multiple Bonds4m
- Multiple Bonds (Simplified)6m
- Lewis Dot Structures: Multiple Bonds10m
- Lewis Dot Structures: Ions (Simplified)8m
- Lewis Dot Structures: Exceptions (Simplified)12m
- Resonance Structures (Simplified)5m
- Valence Shell Electron Pair Repulsion Theory (Simplified)4m
- Electron Geometry (Simplified)8m
- Molecular Geometry (Simplified)11m
- Bond Angles (Simplified)11m
- Dipole Moment (Simplified)15m
- Molecular Polarity (Simplified)7m
- 5. Classification & Balancing of Chemical Reactions3h 17m
- Chemical Reaction: Chemical Change5m
- Law of Conservation of Mass5m
- Balancing Chemical Equations (Simplified)13m
- Solubility Rules16m
- Molecular Equations18m
- Types of Chemical Reactions12m
- Complete Ionic Equations18m
- Calculate Oxidation Numbers15m
- Redox Reactions17m
- Spontaneous Redox Reactions8m
- Balancing Redox Reactions: Acidic Solutions17m
- Balancing Redox Reactions: Basic Solutions17m
- Balancing Redox Reactions (Simplified)13m
- Galvanic Cell (Simplified)16m
- 6. Chemical Reactions & Quantities2h 27m
- 7. Energy, Rate and Equilibrium3h 46m
- Nature of Energy6m
- First Law of Thermodynamics7m
- Endothermic & Exothermic Reactions7m
- Bond Energy14m
- Thermochemical Equations12m
- Heat Capacity19m
- Thermal Equilibrium (Simplified)8m
- Hess's Law23m
- Rate of Reaction11m
- Energy Diagrams12m
- Chemical Equilibrium7m
- The Equilibrium Constant14m
- Le Chatelier's Principle23m
- Solubility Product Constant (Ksp)17m
- Spontaneous Reaction10m
- Entropy (Simplified)9m
- Gibbs Free Energy (Simplified)18m
- 8. Gases, Liquids and Solids3h 25m
- Pressure Units6m
- Kinetic Molecular Theory14m
- The Ideal Gas Law18m
- The Ideal Gas Law Derivations13m
- The Ideal Gas Law Applications6m
- Chemistry Gas Laws16m
- Chemistry Gas Laws: Combined Gas Law12m
- Standard Temperature and Pressure14m
- Dalton's Law: Partial Pressure (Simplified)13m
- Gas Stoichiometry18m
- Intermolecular Forces (Simplified)19m
- Intermolecular Forces and Physical Properties11m
- Atomic, Ionic and Molecular Solids10m
- Heating and Cooling Curves30m
- 9. Solutions4h 10m
- Solutions6m
- Solubility and Intermolecular Forces18m
- Solutions: Mass Percent6m
- Percent Concentrations10m
- Molarity18m
- Osmolarity15m
- Parts per Million (ppm)13m
- Solubility: Temperature Effect8m
- Intro to Henry's Law4m
- Henry's Law Calculations12m
- Dilutions12m
- Solution Stoichiometry14m
- Electrolytes (Simplified)13m
- Equivalents11m
- Molality15m
- The Colligative Properties15m
- Boiling Point Elevation16m
- Freezing Point Depression9m
- Osmosis16m
- Osmotic Pressure9m
- 10. Acids and Bases3h 29m
- Acid-Base Introduction11m
- Arrhenius Acid and Base6m
- Bronsted Lowry Acid and Base18m
- Acid and Base Strength17m
- Ka and Kb12m
- The pH Scale19m
- Auto-Ionization9m
- pH of Strong Acids and Bases9m
- Acid-Base Equivalents14m
- Acid-Base Reactions7m
- Gas Evolution Equations (Simplified)6m
- Ionic Salts (Simplified)23m
- Buffers25m
- Henderson-Hasselbalch Equation16m
- Strong Acid Strong Base Titrations (Simplified)10m
- 11. Nuclear Chemistry56m
- BONUS: Lab Techniques and Procedures1h 38m
- BONUS: Mathematical Operations and Functions47m
- 12. Introduction to Organic Chemistry1h 34m
- 13. Alkenes, Alkynes, and Aromatic Compounds2h 12m
- 14. Compounds with Oxygen or Sulfur1h 6m
- 15. Aldehydes and Ketones1h 1m
- 16. Carboxylic Acids and Their Derivatives1h 11m
- 17. Amines39m
- 18. Amino Acids and Proteins1h 51m
- 19. Enzymes1h 37m
- 20. Carbohydrates1h 41m
- Intro to Carbohydrates4m
- Classification of Carbohydrates4m
- Fischer Projections4m
- Enantiomers vs Diastereomers8m
- D vs L Enantiomers8m
- Cyclic Hemiacetals8m
- Intro to Haworth Projections4m
- Cyclic Structures of Monosaccharides11m
- Mutarotation4m
- Reduction of Monosaccharides10m
- Oxidation of Monosaccharides7m
- Glycosidic Linkage14m
- Disaccharides7m
- Polysaccharides2m
- 21. The Generation of Biochemical Energy2h 8m
- 22. Carbohydrate Metabolism2h 22m
- 23. Lipids2h 26m
- Intro to Lipids6m
- Fatty Acids25m
- Physical Properties of Fatty Acids6m
- Waxes4m
- Triacylglycerols12m
- Triacylglycerol Reactions: Hydrogenation8m
- Triacylglycerol Reactions: Hydrolysis13m
- Triacylglycerol Reactions: Oxidation7m
- Glycerophospholipids15m
- Sphingomyelins13m
- Steroids15m
- Cell Membranes7m
- Membrane Transport10m
- 24. Lipid Metabolism1h 45m
- 25. Protein and Amino Acid Metabolism1h 37m
- 26. Nucleic Acids and Protein Synthesis2h 54m
- Intro to Nucleic Acids4m
- Nitrogenous Bases16m
- Nucleoside and Nucleotide Formation9m
- Naming Nucleosides and Nucleotides13m
- Phosphodiester Bond Formation7m
- Primary Structure of Nucleic Acids11m
- Base Pairing10m
- DNA Double Helix6m
- Intro to DNA Replication20m
- Steps of DNA Replication11m
- Types of RNA10m
- Overview of Protein Synthesis4m
- Transcription: mRNA Synthesis9m
- Processing of pre-mRNA5m
- The Genetic Code6m
- Introduction to Translation7m
- Translation: Protein Synthesis18m
Standard Temperature and Pressure: Videos & Practice Problems
Standard temperature and pressure (STP) is defined as a temperature of 273.15 Kelvin (0 degrees Celsius) and a pressure of 1 atmosphere. At STP, the standard molar volume of an ideal gas is 22.4 liters, which establishes a crucial relationship between moles and volume. The equation for volume is given by , where V is volume, n is moles, R is the gas constant, T is temperature, and P is pressure.
In order to accurately study the effect that changes in pressure, temperature and moles have on volume, chemists will often run their experiments under Standard Temperature and Pressure conditions.
Standard Temperature and Pressure
Standard Temperature and Pressure Video Summary
Standard Temperature and Pressure Example 1
Standard Temperature and Pressure Example 1 Video Summary
To determine the mass of oxygen gas present in a sample with a volume of 325 mL at standard temperature and pressure (STP), we can utilize the ideal gas law. At STP, the pressure is 1 atmosphere, and the temperature is 273.15 Kelvin. The ideal gas law can be expressed as:
$$ n = \frac{PV}{RT} $$
Where:
- n = number of moles
- P = pressure (1 atm)
- V = volume in liters (0.325 L)
- R = ideal gas constant (0.08206 L·atm/(mol·K))
- T = temperature in Kelvin (273.15 K)
First, convert the volume from milliliters to liters:
$$ V = 325 \, \text{mL} = 0.325 \, \text{L} $$
Next, substitute the values into the equation to find the number of moles:
$$ n = \frac{(1 \, \text{atm})(0.325 \, \text{L})}{(0.08206 \, \text{L·atm/(mol·K)})(273.15 \, \text{K})} $$
Calculating this gives:
$$ n \approx 0.01450 \, \text{moles of } O_2 $$
To convert moles to grams, use the molar mass of oxygen gas (O2), which is 32 grams per mole:
$$ \text{mass} = n \times \text{molar mass} $$
$$ \text{mass} = 0.01450 \, \text{moles} \times 32 \, \text{g/mol} $$
This results in:
$$ \text{mass} \approx 0.464 \, \text{grams of } O_2 $$
When considering significant figures, the final answer should reflect three significant figures, resulting in:
$$ \text{mass} \approx 0.464 \, \text{grams of } O_2 $$
In summary, by applying the ideal gas law and converting moles to grams, we find that a sample of oxygen gas with a volume of 325 mL at STP contains approximately 0.464 grams of O2.
Standard Temperature and Pressure
Standard Temperature and Pressure Video Summary
In the context of standard temperature and pressure (STP), the concept of standard molar volume is crucial for understanding the behavior of gases. Standard molar volume refers to the volume occupied by one mole of an ideal gas at STP, which is defined as a temperature of 273.15 Kelvin and a pressure of 1 atmosphere.
The relationship between volume, moles, and the ideal gas law can be expressed with the formula:
V = n \cdot \frac{RT}{P}
In this equation, V represents volume, n is the number of moles, R is the ideal gas constant, T is the temperature in Kelvin, and P is the pressure in atmospheres. When we consider 1 mole of an ideal gas at STP, the moles cancel out, and we can simplify the equation to find the volume:
V = \frac{RT}{P}
Substituting the values for R (0.0821 L·atm/(K·mol)), T (273.15 K), and P (1 atm), we find that the volume is:
V = 0.0821 \cdot 273.15 / 1 = 22.4 \text{ liters}
This result indicates that the standard molar volume of an ideal gas at STP is 22.4 liters. This value serves as a vital conversion factor, allowing for the conversion between moles and volume for any ideal gas under these conditions. Therefore, whenever dealing with 1 mole of an ideal gas at STP, one can confidently use the standard molar volume of 22.4 liters.
Standard Temperature and Pressure Example 2
Standard Temperature and Pressure Example 2 Video Summary
To determine the number of moles of chlorine gas (Cl2) occupying a volume of 15.7 liters at standard temperature and pressure (STP), we can utilize two different methods based on the principles of gas laws.
The first method involves using the standard molar volume of an ideal gas, which is 22.4 liters per mole at STP. By applying this conversion factor, we can calculate the moles of Cl2 as follows:
Given:
Volume (V) = 15.7 liters
Conversion factor = 1 mole / 22.4 liters
Calculating moles:
moles = 15.7 liters × (1 mole / 22.4 liters) = 0.701 moles of Cl2
The second method employs the ideal gas law, represented by the equation:
PV = nRT
Where:
- P = pressure (1 atmosphere at STP)
- V = volume (15.7 liters)
- n = number of moles
- R = ideal gas constant (0.0821 L·atm/(K·mol))
- T = temperature (273.15 K at STP)
Rearranging the equation to solve for n gives:
n = PV / RT
Substituting the known values:
n = (1 atm) × (15.7 L) / (0.0821 L·atm/(K·mol) × 273.15 K)
Calculating this yields:
n ≈ 0.701 moles of Cl2
Both methods yield the same result, demonstrating that we can determine the number of moles of a gas at STP either through the standard molar volume or by applying the ideal gas law. Understanding these approaches is essential for solving gas-related problems in chemistry.
A sample of dichloromethane gas (CH2Cl2) occupies 32.6 L at 310 K and 5.30 atm. Determine its volume at STP?
Which gas sample has the greatest volume at STP?
Nitrogen and hydrogen combine to form ammonia via the following reaction:
1 N2 (s) + 3 H2 (g) → 2 NH3 (g)
What mass of nitrogen is required to completely react with 800.0 mL H2 at STP?
Do you want more practice?
Here’s what students ask on this topic:
What is the definition of Standard Temperature and Pressure (STP)?
Standard Temperature and Pressure (STP) is a reference point used in gas calculations. It is defined as a temperature of 273.15 Kelvin (0 degrees Celsius) and a pressure of 1 atmosphere. These conditions are used to standardize measurements and calculations involving gases, making it easier to compare different sets of data. At STP, the standard molar volume of an ideal gas is 22.4 liters, which helps establish a relationship between moles and volume.
How do you calculate the volume of a gas at STP?
To calculate the volume of a gas at STP, you can use the ideal gas law equation: . Here, is the volume, is the number of moles, is the gas constant, is the temperature in Kelvin, and is the pressure in atmospheres. At STP, is 273.15 K and is 1 atm. For 1 mole of an ideal gas, the volume is 22.4 liters.
What is the standard molar volume of an ideal gas at STP?
The standard molar volume of an ideal gas at STP is 22.4 liters. This means that one mole of any ideal gas occupies 22.4 liters of volume when the temperature is 273.15 Kelvin (0 degrees Celsius) and the pressure is 1 atmosphere. This value is derived from the ideal gas law and is a useful conversion factor in gas calculations.
Why is STP important in gas calculations?
STP is important in gas calculations because it provides a standardized set of conditions (273.15 K and 1 atm) that allow for consistent and comparable measurements. Using STP, scientists and engineers can easily compare the properties of different gases and perform calculations involving gas volumes, pressures, and temperatures. The standard molar volume of 22.4 liters at STP also simplifies the relationship between moles and volume, making it easier to convert between these quantities.
How does the ideal gas law relate to STP?
The ideal gas law, given by the equation , relates pressure (P), volume (V), moles of gas (n), the gas constant (R), and temperature (T). At STP, the temperature is 273.15 K and the pressure is 1 atm. By substituting these values into the ideal gas law, we can determine the volume of one mole of an ideal gas, which is 22.4 liters. This relationship helps in understanding and predicting the behavior of gases under standard conditions.