Overview

Mars is the fourth terrestrial (or rocky) planet from the sun and Earth's closest planetary neighbor, at an average distance of 225 million kilometers. It is about half the size of Earth, contains a fraction of its atmosphere, and has two irregularly shaped moons: Phobos and Deimos.

1440 Findings

Hours of research by our editors, distilled into minutes of clarity.

  • Mars once had oceans and a thick atmosphere

    It formed over millions of years as small clumps of matter orbiting the sun smashed together, solidified, and cooled. Geological features indicate the presence of past surface water, which evaporated away due to the planet's weak gravitational field.

  • Explore the Spirit and Opportunity Martian rovers

    The twin machines were tasked with studying the geology of Mars to identify evidence of past water activity, determine the composition of minerals, rocks, and soils, and perform "ground truth" experiments to calibrate and validate observations made by Mars orbiters.

  • Solar wind may have contributed to Mars losing its atmosphere

    Scientists believe that over hundreds of millions of years, energetic particles from the sun colliding with atmospheric particles, flinging them away from Mars' weak gravitational field like colliding billiard balls. As atmospheric pressure decline, water also evaporated away from the surface.

  • Explore a world map of Mars

    The yellows spots scattered across the map indicate meteor impacts while the red regions represent volcanoes and their associated lava flows. The varying shades of brown indicate cratered highlands and midlands, which make up most of the southern hemisphere.

  • From the surface, Mars can appear butterscotch, golden brown, and even green

    Images from orbiters, landers, and rovers show that Mars has a mix of surface colors resulting from variations in the mineral compositions of different regions. The reddish tint when viewed from Earth comes from kicked up particles of rusted iron.

  • While geography pertains to Earth's surface features, areography pertains to Mars

    Unlike Earth, Mars lacks geological activity and oceans, though geological evidence suggests they both existed in the past. Its northern regions have far fewer craters than the southern ones, indicating that the rock in the north formed more recently.

  • Inhabiting Mars without terraforming might be accomplished with 'worldhouses'

    A network of interconnected, airtight bubbles would require several orders of magnitude fewer materials than those required to re-establish the entire planet's atmosphere to resemble Earth. However, the whole network would be compromised by a single micrometeor impact that destroys the air seal.

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