MESSENGER Confirms Water Ice and Organic Material on Mercury

New data obtained with NASA’s MESSENGER spacecraft have provided evidence that water ice and deposits of organic material exist near the north pole of Mercury.

This is a temperature map of the north polar region of Mercury, calculated at the University of California in Los Angeles using topographic data collected by NASA’s MESSENGER spacecraft (NASA / UCLA / JHUAPL / Carnegie Institution of Washington)

In the early 1990s, scientists were surprised to find that areas near Mercury’s poles were unusually bright when observed with radar from Earth, a potential indication that ice might be present.

Mercury is the innermost planet in the Solar system, and, arguably, it’s among the least explored. The surface of Mercury exhibits the most extreme range of temperatures of any body we know of in the Solar system,” said Dr David Paige of the University of California in Los Angeles, lead author of one of three new MESSENGER papers published in the journal Science.

“Within a single polar crater on Mercury, there are spots that reach the oven-like temperature of 500 degrees Fahrenheit within sight of areas cold enough to freeze and preserve water ice for billions of years. These natural freezers exist within the shadowed areas of polar-crater rims, which never experience direct sunlight due to the low angle of the Sun at such high latitudes,” he said.

Dr Paige’s team has used detailed topographic map of Mercury’s north polar region produced by MESSENGER to generate an accurate thermal model of the pole. Their calculations of the planet’s sub-surface temperatures are a near-perfect match to Earth-based radar observations and surface-brightness measurements made by the MESSENGER’s Mercury Laser Altimeter (MLA).

Where their temperature model predicts water ice should be stable on the surface, the MLA nearly always measures unusually bright patches, indicative of surface ice deposits. In places where it is too warm for surface ice but cold enough for ice to exist beneath the surface, the MLA sees unusually dark material.

“This stuff we find covering the ice is darker than the rest of Mercury, which is already a really dark planet. That’s amazing,” Dr Paige said. “At the very least, it means there is something out of the ordinary going on inside these permanently shadowed areas where the ice has accumulated. The mysterious dark substance likely arrived on Mercury as part of the comets and asteroids that periodically crash into the planet, bringing water ice and a diverse cocktail of organic material. In the searing daytime heat of Mercury, the only place water and organics can survive is within permanently shadowed craters.”

But only in the very coldest areas of the permanently shadowed regions can water ice exist on the surface. In the warmer shadowed areas, the top layers of ice begin to evaporate away into space, leaving behind a layer of hardy organic molecules that are stable at higher temperatures and which turn black over time when exposed at the surface. Once the dark layer is thick enough, it protects the ice underneath, allowing a sub-surface ice deposit to survive.

“There are areas on the surface where it is too hot for ice to exist, but radar data from Earth show something bright reflecting from these areas, so we’re pretty sure that there’s water ice buried underneath,” said co-author Dr Matthew Siegler of the Jet Propulsion Laboratory. “You need some kind of insulating layer to keep that heat from getting down to the ice.”

The presence of bright ice and dark organics on Mercury’s surface presents a mystery for MESSENGER researchers. Large comets and asteroids periodically impact Mercury, covering a huge swath of the planet in a layer of dirt and dust and adding further craters to the airless planet’s already scarred landscape. For the water ice and black organic layers to remain exposed on Mercury’s ancient surface, the deposits must have formed recently in the planet’s geological history, or they must be maintained by new water brought to Mercury by smaller, more frequent impacts.

“Billions of years ago, the Earth acquired a layer of water and other volatile material that formed atmospheres, oceans and even the first organic molecules that started life,” Dr Paige said. “Understanding the origin of that material is a very important problem and is essential to finding out about the potential habitability of planetary systems around other stars.”


Bibliographic information: David A. Paige et al. Thermal Stability of Volatiles in the North Polar Region of Mercury. Science, published online November 29, 2012; doi: 10.1126/science.1231106