Mercury harbors water ice in the shadows of the steepest craters around its poles. But it is unclear how those water molecules ended up on Mercury. Now a new simulation shows that incoming minor bodies such as asteroids, comets and dust particles carry enough water to account for all the ice sheets present. The study could form the basis for new research on water in exoplanetary systems. Publication in Icarus on April 19th.
ice on mercury
We have known for a few decades that Mercury harbors water. You might expect that this can only be in the form of water vapor. After all, the planet has no atmosphere so we can rule out a liquid due to a lack of pressure. And Mercury is almost three times closer to the Sun than the Earth is, so water ice doesn’t seem likely either. But then you forgot about craters. Steep craters at high latitudes contain troughs that are forever captured in darkness, only illuminated by the dimly glowing band of the Milky Way against the backdrop of an eternal black sky. These eerie places are home to ice sheets many meters thick, on the closest planet to the Sun. Now the question remains: how did those water molecules end up on Mercury?
simulation for meteorite impacts
First author Kateryna Frantseva (SRON/RUG) has developed an algorithm that simulates meteorite impacts in the form of asteroids, comets and interplanetary dust particles (IDPs). It turns out that over the course of a billion years these bodies bring enough water to Mercury’s surface to explain the amount that we currently see.
ten thousand kilograms of dust particles
Frantseva: ‘We cannot rule out endogenous sources of water such as volcanic activity and outgassing from the crust and mantle, but this shows that we don’t need anything other than impacts from minor bodies to explain the water we see on Mercury.’ The simulation shows that IDPs carry by far the heaviest load, with over ten thousand kilograms per year. In comparison, asteroids and comets deliver yearly each about a thousand kilograms.
water delivery to exoplanets
The simulation provides a basis for new theoretical models for water delivery to exoplanets—planets outside our Solar System. These can be compared to future observations, for example from the recently launched James Webb telescope, in which astronomers might be able to spot water signatures in the spectrum of light that asteroid belts in exoplanetary systems emit while re-radiating light from their host star.
First author Kateryna Frantseva is a Ukrainian scientist based in The Netherlands. She is part of a network of Ukrainian volunteers working in Dutch academia that support their home country. To help out, you can donate here. If you live outside of The Netherlands, you can donate here. The cartoon was made by Anastasiia Kriuchevska.