Iron oxide gives the Red Planet its distinctive hue, but why is there so much iron on the surface? And how did it oxidize?
The simple explanation for the Red Planet's color is that its regolith, or surface material, contains lots of iron oxide — the same compound that gives blood and rust their hue. But why does Mars have so much iron, why is that iron "oxidized," and why does iron oxide look red?
It all started 4.5 billion years ago. When the solar system formed, many of the planets landed a dose of iron. Forged in the heart of long-dead stars, the heavy element swirled around in the cloud of gas and dust that gravitationally collapsed to form the sun and planets. Whereas the bulk of Earth's iron sank to its core when the planet was young and molten, NASA scientists think Mars' smaller size (and weaker gravity) allowed it to remain less differentiated. It does have an iron core, but abundant iron exists in its upper layers, also.
Plain-old iron looks shiny black. The element only takes on a reddish tinge when it has been exposed to oxygen, and enough oxygen at that for it to become iron(III) oxide, an atomic fivesome composed of two iron atoms and three oxygen atoms. So why did so much of the iron on Mars' surface oxidize, or gang up with oxygen?
In fact, the jury's still out on that one. For sure, some sort of weathering gradually rusted the iron on Mars. But did the ancient rainstorms that are thought to have occurred on a young, wet Mars rust the iron by pounding the regolith with oxygen atoms freed from water molecules? Or, did the oxidation happen gradually over billions of years, as sunlight broke down carbon dioxide and other molecules in the atmosphere, producing oxidants such as hydrogen peroxide and ozone? Or, as a group of Danish scientists suggested in 2009, have Martian dust storms slowly rusted the iron, by crumbling the quartz crystals that also exist in the regolith and leaving their oxygen-rich surfaces exposed?