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MARS WEATHER

Mars Weather: Temperature, Pressure and Wind

Mars weather is a highly variable combination of extreme cold, low atmospheric pressure, wind and airborne dust. This page connects the latest available station observations to modelled regional context without presenting forecasts as direct measurements.

Surface-temperature ranges, atmospheric pressure and wind estimates are shown with their site, time and evidence class. A value marked as observed comes from a published mission record; a model value describes regional conditions rather than an instrument reading.

Latitude, elevation, local solar time, season and dust loading all affect conditions. Mars also has a thin atmosphere and a large day-night temperature range, so a single global number cannot describe the planet.

Use the timestamp and source class before comparing sites. Direct observations, climatological products and operational estimates answer different questions and should not be merged into one unqualified weather value.

Global view of Mars
NASA/USGS scientific context image; consult the cited source for product-level attribution.

Scientific dossier

A planet with weather, seasons and dust

Martian weather is governed by a thin carbon-dioxide atmosphere, a large daily thermal cycle, seasonal exchange with the polar caps and dust that changes heating across the planet. Scientific interpretation therefore begins with place, sol, local solar time and evidence class.

From telescopes to surface stations

Seasonal markings and dust were first followed from Earth. Mariner and Viking established planetary meteorology; later orbiters mapped clouds, water vapour and dust, while landers and rovers measured local pressure, temperature, wind and radiation.

Temperature, pressure and circulation

Mars can be comparatively mild on sunlit equatorial ground and extremely cold at night and near the poles. Pressure is less than one percent of Earth's mean sea-level pressure and varies with elevation and seasonal carbon-dioxide frost.

Observation versus model

A rover observation applies to its instrument, site and published sol. A climatological field estimates conditions beyond the station network. Retrieval time, observation time and model epoch are therefore published separately.

Evidence standard

From registered source to published evidence

Status semantics

Registered identifies a source in the catalogue. Monitored confirms endpoint availability. Discovered marks a candidate release. Ingested means a record has entered the normalized research corpus.

Scientific boundary

Terrain values derive from published planetary datasets. Atmospheric values are climatological estimates unless explicitly labelled as rover observations. Coordinates select a comparative model context rather than a local weather station.

Uncertainty

Displayed ranges communicate model envelopes and source limitations. They must not be read as instrument error bars or real-time forecasts at arbitrary coordinates.

Primary records

The source register connects NASA PDS, ESA PSA, USGS Astrogeology, rover archives, MOLA relief products, and peer-reviewed planetary research.