Earth ScienceGeology & MeteorologyMedium

Atmosphere (Earth)

Also known as:air massEarth's air envelopegaseous envelope

The Earth's atmosphere is the layer of gases retained by Earth's gravity surrounding the planet, extending from the surface to approximately 10,000 km altitude where it gradually merges with the interplanetary medium. It consists primarily of nitrogen (78.09%), oxygen (20.95%), argon (0.93%), and carbon dioxide (0.04%), plus trace gases and variable amounts of water vapor. The atmosphere performs critical functions including regulating surface temperature through the greenhouse effect, protecting life from harmful ultraviolet radiation via the ozone layer, enabling weather and climate systems, and providing the oxygen and carbon dioxide essential for respiration and photosynthesis.

Key Formula

P = P0 × e^(−Mgh/RT)

LaTeX: P = P_0 \, e^{-Mgh/RT}

SymbolMeaningUnit
PAtmospheric pressure at altitude hPa
P_0Sea-level atmospheric pressure (101,325 Pa)Pa
MMolar mass of air (0.02896 kg/mol)kg/mol
gGravitational acceleration (9.81 m/s²)m/s²
hAltitude above sea levelm
RUniversal gas constant (8.314 J/mol·K)J/(mol·K)
TTemperatureK

Worked Example

Problem

Calculate the atmospheric pressure at an altitude of 5,000 m above sea level, assuming a constant temperature of 255 K (isothermal approximation). Use P₀ = 101,325 Pa, M = 0.02896 kg/mol, g = 9.81 m/s², R = 8.314 J/(mol·K).

Solution

Step 1: Calculate the exponent. Exponent = −Mgh/RT = −(0.02896 × 9.81 × 5000) / (8.314 × 255) = −(1421.4) / (2120.1) = −0.6705 Step 2: Evaluate the exponential. e^(−0.6705) ≈ 0.5114 Step 3: Calculate pressure. P = 101,325 × 0.5114 ≈ 51,807 Pa ≈ 51.8 kPa

Answer

Approximately 51.8 kPa (about 51% of sea-level pressure)

Composition of Earth's Dry Atmosphere

GasChemical SymbolVolume Fraction (%)RoleTrend
NitrogenN₂78.09Diluent, nutrient cycleStable
OxygenO₂20.95Respiration, combustionStable
ArgonAr0.93Inert fillerStable
Carbon dioxideCO₂0.042Greenhouse gas, photosynthesisIncreasing (~3 ppm/yr)
MethaneCH₄0.000187Potent greenhouse gasIncreasing
OzoneO₃0.000006UV shield in stratosphereRecovering

Interactive Tools

NASA Goddard: Atmosphere Overview

Open Tool

Khan Academy: Earth's Atmosphere

Open Tool

Wolfram Alpha: Barometric Formula

Open Tool
Diagram of Earth's atmospheric layers from troposphere to exosphere with altitude and temperature profiles

Wikimedia Commons, CC BY-SA

Related Terms

Earth Science

Troposphere

The troposphere is the lowest layer of Earth's atmosphere, extending from the surface to approximately 8–9 km at the poles and 16–18 km at the equator, and containing about 80% of the atmosphere's total mass and virtually all of its water vapor and weather. Temperature generally decreases with altitude at the environmental lapse rate of approximately 6.5°C per 1,000 m (the standard atmosphere value), until reaching the tropopause, a temperature inversion that caps the troposphere. All significant weather phenomena — clouds, precipitation, thunderstorms, cyclones, and jet streams — occur within the troposphere, making it the most meteorologically active layer.

Earth Science

Stratosphere

The stratosphere is the second major layer of Earth's atmosphere, extending from the tropopause (approximately 12 km at mid-latitudes) to the stratopause at about 50 km altitude. Unlike the troposphere, temperature in the stratosphere increases with altitude — from about −56°C at the tropopause to approximately 0°C at the stratopause — due to the absorption of ultraviolet radiation by the ozone layer concentrated within it. This temperature inversion creates very stable conditions that suppress vertical mixing, making the stratosphere nearly cloud-free and home to the polar vortex and stratospheric jet streams; it is also the layer traversed by high-altitude commercial aircraft.

Earth Science

Ozone Layer

The ozone layer is a region of Earth's stratosphere, concentrated approximately 15–35 km above the surface, where ozone (O₃) molecules are present at relatively high concentrations (2–8 ppm), absorbing 97–99% of the Sun's medium-frequency ultraviolet radiation. Ozone is continuously formed when UV radiation (wavelength < 240 nm) splits O₂ molecules into oxygen atoms that then react with other O₂ molecules, and destroyed by catalytic cycles involving chlorine, bromine, nitrogen, and hydrogen radicals. Depletion of the ozone layer by synthetic chlorofluorocarbons (CFCs) — culminating in the discovery of the Antarctic ozone hole in 1985 — led to the Montreal Protocol (1987), which has successfully reduced stratospheric chlorine loading and begun the layer's recovery.

From Greek "atmos" (vapor, steam) and "sphaira" (sphere, globe). The term was coined in the 17th century; it appears in scientific literature by 1638 (John Wilkins) and was used by Edmond Halley and others to describe the gaseous envelope of Earth. The concept that air has weight and pressure was established by Evangelista Torricelli in 1643.

atmospheremeteorologyclimategreenhouse-effectcomposition-of-air