September 6, 2019
Next year, both NASA and the European Space Agency (ESA) will send new rovers to Mars to hunt for evidence of past life.
As previous missions have discovered, Mars had a warmer and wetter past, featuring conditions that could probably sustain life. Current satellites orbiting Mars also reveal there are many places where water was once present on the surface.
The difficulty in hunting for life lies not in finding where there was water, but in identifying where the essential nutrients for life coincided with water.
Micrometeorites mean potential life
For life to move into a new environment and survive, it needs essential nutrients such as carbon, hydrogen, nitrogen, oxygen, phosphorus, and sulfur (together known as CHNOPS), plus other trace elements. It also needs to acquire energy from the environment. Some of Earth’s earliest life forms gained energy by oxidising minerals.
Mars’s crust is mostly made of intrusive and volcanic basalt (the same rock that forms from Hawaii’s lavas) which is not particularly nutrient-rich. However, meteorites and micrometeorites are known to continuously provide essential nutrients to the surfaces of planets.
Our team investigated how much cosmic dust (comet and asteroid dust) would survive atmospheric entry to Mars, and where it would accumulate on the surface as micrometeorites.
We modelled the heating and oxidation effects of atmospheric entry to Mars and found most particles less than about 0.1-0.2mm in diameter would not melt, depending on their composition. In terms of materials accumulating on the martian surface, particles of this size are overwhelmingly more common than larger particles.
On Earth, about 100 times as much cosmic dust in this size range accumulates on the surface, when compared to meteorites larger than 4mm. This is despite extensive melting and evaporation during atmospheric entry to Earth.
Evidence closer to home
As part of our research, we used an analogue site on the Nullarbor Plain in South Australia (which, like Mars, has wind-modified sediment sitting on cracked bedrock) to examine whether wind causes micrometeorites to accumulate at predictable locations.
We found more than 1,600 micrometeorites from a variety of sample sites.
Our observations show that because many micrometeorites are denser than normal sand grains, they are likely to accumulate in bedrock cracks and on gravel-rich surfaces where lighter particles have been blown away. Our samples typically contained several hundred micrometeorites per kilogram.
Several factors added together indicate that micrometeorites should be much more abundant on Mars than on Earth. And this is expected to be true for most of Mars’s 4.5-billion-year history.
Even martians need nutrients
Unmelted and partially melted micrometeorites supply complex carbon compounds to the martian surface, which are the building blocks of life. They also supply the only source of reduced phosphorus through the mineral schreibersite, which has been shown to react with simple hydroxyl compounds to form the precursors for life.
Micrometeorites also provide other reduced minerals like sulfides and iron-nickel metal that can be exploited as an energy source by primitive microbes. Therefore, they provide both the essential nutrients and an energy source that can allow existing microbes to migrate and persist.
Many scientists believe life on Earth may have started around undersea geothermal vents or in volcanic hot springs like those at Yellowstone or Rotorua. Beneath these, water circulates through the hot crust, dissolving nutrients from the rocks and carrying them upwards to the vents, where there are dramatic changes in temperature and chemistry.
Cover image via NASA
Source: The Conversation