MODULE:KNOWLEDGE-BASE
SIMULATION: ACTIVE
RETURN::Planetary Science

Atmospheres

Composition, Pressure & the Greenhouse Effect

Atmospheric Comparison

Atmospheric thickness shown is exaggerated 3–5× relative to body radius for visibility — Earth's real atmosphere is paper-thin against the planet. Cloud motion reflects relative super-rotation rates.

Anatomy of an Atmosphere

Pressure falls off exponentially with altitude. The scale height H = kT/(mg) is the altitude at which pressure drops by a factor of e — determined by temperature, gas mass, and gravity.

Layers from surface outward: troposphere (weather), stratosphere (ozone, jet streams), mesosphere, thermosphere (auroras), and the diffuse exosphere bleeding into space.

Whether a planet keeps its atmosphere depends on escape velocity versus molecular thermal speeds — light gases like H₂ leak from any terrestrial body, heavy gases like CO₂ stay put.

Greenhouse & Climate
MarsThin CO₂ — weak greenhouse, freezes despite sunlight
EarthTrace CO₂/H₂O — +33 °C of warming over no-atmosphere baseline
TitanCH₄ greenhouse + N₂ pressure-broadening
VenusRunaway: 96% CO₂ → +500 °C of greenhouse forcing

The same physics drives why ELWs are rare — small composition shifts run away in either direction.

ED: Atmospheric Landings

Odyssey introduced landings on bodies with thin atmospheres only — typically pressure under ~0.1 atm. Anything thicker remains no-land.

The system map flags atmospheric type on every body. Common atmospheric compositions in ED: CO₂, SO₂, water, methane, ammonia, helium, and neon. Atmosphere composition is a scan-bonus parameter.

Look for N₂/O₂ on a non-ELW: it usually flags a terraformable body with substantial cartographic value.

Atmosphere Reference — Sol System
BodySurface PCompositionScale HSurface TNote
Mercury10⁻¹⁵ atmTrace He, Na, K (exosphere only)−180 / +430 °CEffectively no atmosphere
Mars0.006 atm95% CO₂, 3% N₂, 1.6% Ar11 km−63 °C avgThin, dust storms, no greenhouse
Earth1.0 atm78% N₂, 21% O₂, 1% Ar/H₂O8.5 km+15 °C avgLiquid water, biosphere, magnetic field
Titan1.45 atm95% N₂, 5% CH₄, ethane haze50 km−179 °CThickest moon atmosphere; methane cycle
Venus92 atm96% CO₂, 3.5% N₂, H₂SO₄ clouds16 km+462 °CRunaway greenhouse, super-rotation 60×
Jupiter (1 bar)no surface~90% H₂, 10% He, NH₃ clouds27 km−108 °C @ 1 barAtmosphere extends to metallic H mantle
Neptune (1 bar)no surface~80% H₂, 19% He, 1.5% CH₄20 km−201 °C @ 1 barMethane absorption gives blue colour